Sample records for carnegie hubble program

  1. The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using Only Population II Distance Indicators

    NASA Astrophysics Data System (ADS)

    Beaton, Rachael L.; Freedman, Wendy L.; Madore, Barry F.; Bono, Giuseppe; Carlson, Erika K.; Clementini, Gisella; Durbin, Meredith J.; Garofalo, Alessia; Hatt, Dylan; Jang, In Sung; Kollmeier, Juna A.; Lee, Myung Gyoon; Monson, Andrew J.; Rich, Jeffrey A.; Scowcroft, Victoria; Seibert, Mark; Sturch, Laura; Yang, Soung-Chul

    2016-12-01

    We present an overview of the Carnegie-Chicago Hubble Program, an ongoing program to obtain a 3% measurement of the Hubble constant (H 0) using alternative methods to the traditional Cepheid distance scale. We aim to establish a completely independent route to H 0 using RR Lyrae variables, the tip of the red giant branch (TRGB), and Type Ia supernovae (SNe Ia). This alternative distance ladder can be applied to galaxies of any Hubble type, of any inclination, and, using old stars in low-density environments, is robust to the degenerate effects of metallicity and interstellar extinction. Given the relatively small number of SNe Ia host galaxies with independently measured distances, these properties provide a great systematic advantage in the measurement of H 0 via the distance ladder. Initially, the accuracy of our value of H 0 will be set by the five Galactic RR Lyrae calibrators with Hubble Space Telescope Fine-Guidance Sensor parallaxes. With Gaia, both the RR Lyrae zero-point and TRGB method will be independently calibrated, the former with at least an order of magnitude more calibrators and the latter directly through parallax measurement of tip red giants. As the first end-to-end “distance ladder” completely independent of both Cepheid variables and the Large Magellanic Cloud, this path to H 0 will allow for the high-precision comparison at each rung of the traditional distance ladder that is necessary to understand tensions between this and other routes to H 0. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs #13472 and #13691.

  2. The Carnegie Hubble Program: The Leavitt Law at 3.6 microns and 4.5 microns in the Large Magellanic Cloud

    NASA Technical Reports Server (NTRS)

    Scowcroft, Victoria; Freedman, Wendy L.; Madore, Barry F.; Monson, Andrew J.; Persson, S. E.; Seibert, Mark; Rigby, Jane R.; Sturch, Laura

    2011-01-01

    The Carnegie Hubble Program (CHP) is designed to improve the extragalactic distance scale using data from the post-cryogenic era of Spitzer. The ultimate goal is a determination of the Hubble constant to an accuracy of 2%. This paper is the first in a series on the Cepheid population of the Large Magellanic Cloud, and focuses on the period-luminosity relations (Leavitt laws) that will be used, in conjunction with observations of Milky Way Cepheids, to set the slope and zero-point of the Cepheid distance scale in the mid-infrared. To this end, we have obtained uniformly-sampled light curves for 85 LMC Cepheids, having periods between 6 and 140 days. Period- luminosity and period-color relations are presented in the 3.6 micron and 4.5 micron bands. We demonstrate that the 3.6 micron band is a superb distance indicator. The cyclical variation of the [3.6]-[4.5] color has been measured for the first time. We attribute the amplitude and phase of the color curves to the dissociation and recombination of CO molecules in the Cepheid s atmosphere. The CO affects only the 4.5 micron flux making it a potential metallicity indicator.

  3. The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period-luminosity Relations

    NASA Astrophysics Data System (ADS)

    Hatt, Dylan; Beaton, Rachael L.; Freedman, Wendy L.; Madore, Barry F.; Jang, In-Sung; Hoyt, Taylor J.; Lee, Myung Gyoon; Monson, Andrew J.; Rich, Jeffrey A.; Scowcroft, Victoria; Seibert, Mark

    2017-08-01

    IC 1613 is an isolated dwarf galaxy within the Local Group. Low foreground and internal extinction, low metallicity, and low crowding make it an invaluable testbed for the calibration of the local distance ladder. We present new, high-fidelity distance estimates to IC 1613 via its Tip of the Red Giant Branch (TRGB) and its RR Lyrae (RRL) variables as part of the Carnegie-Chicago Hubble Program, which seeks an alternate local route to H 0 using Population II stars. We have measured a TRGB magnitude {I}{ACS}{TRGB}=20.35+/- {0.01}{stat}+/- {0.01}{sys} mag using wide-field observations obtained from the IMACS camera on the Magellan-Baade telescope. We have further constructed optical and near-infrared RRL light curves using archival BI- and new H-band observations from the ACS/WFC and WFC3/IR instruments on board the Hubble Space Telescope (HST). In advance of future Gaia data releases, we set provisional values for the TRGB luminosity via the Large Magellanic Cloud and Galactic RRL zero-points via HST parallaxes. We find corresponding true distance moduli {μ }0{TRGB}=24.30+/- {0.03}{stat}+/- {0.05}{sys} {mag} and < {μ }0{RRL}> =24.28+/- {0.04}{stat+{sys}} mag. We compare our results to a body of recent publications on IC 1613 and find no statistically significant difference between the distances derived from Population I and II stars. Based in part on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs #10505 and #13691. Additional observations are credited to the Observatories of the Carnegie Institution of Washington for the use of Magellan-Baade IMACS. Presented as part of a dissertation to the Department of Astronomy and Astrophysics, The University of Chicago, in partial fulfillment of the requirements for the Ph.D. degree.

  4. The Carnegie-Chicago Hubble Program: Discovery of the Most Distant Ultra-faint Dwarf Galaxy in the Local Universe

    NASA Astrophysics Data System (ADS)

    Lee, Myung Gyoon; Jang, In Sung; Beaton, Rachael; Seibert, Mark; Bono, Giuseppe; Madore, Barry

    2017-02-01

    Ultra-faint dwarf galaxies (UFDs) are the faintest known galaxies, and due to their incredibly low surface brightness, it is difficult to find them beyond the Local Group. We report a serendipitous discovery of a UFD, Fornax UFD1, in the outskirts of NGC 1316, a giant galaxy in the Fornax cluster. The new galaxy is located at a projected radius of 55 kpc in the south-east of NGC 1316. This UFD is found as a small group of resolved stars in the Hubble Space Telescope images of a halo field of NGC 1316, obtained as part of the Carnegie-Chicago Hubble Program. Resolved stars in this galaxy are consistent with being mostly metal-poor red giant branch (RGB) stars. Applying the tip of the RGB method to the mean magnitude of the two brightest RGB stars, we estimate the distance to this galaxy, 19.0 ± 1.3 Mpc. Fornax UFD1 is probably a member of the Fornax cluster. The color-magnitude diagram of these stars is matched by a 12 Gyr isochrone with low metallicity ([Fe/H] ≈ -2.4). Total magnitude and effective radius of Fornax UFD1 are MV ≈ -7.6 ± 0.2 mag and reff = 146 ± 9 pc, which are similar to those of Virgo UFD1 that was discovered recently in the intracluster field of Virgo by Jang & Lee. Fornax UFD1 is the most distant known UFD that is confirmed by resolved stars. This indicates that UFDs are ubiquitous and that more UFDs remain to be discovered in the Fornax cluster. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs #10505 and #13691.

  5. The Carnegie Hubble Program

    NASA Technical Reports Server (NTRS)

    Freedman, Wendy L.; Madore, Barry F.; Scowcroft, Vicky; Mnso, Andy; Persson, S. E.; Rigby, Jane; Sturch, Laura; Stetson, Peter

    2011-01-01

    We present an overview of and preliminary results from an ongoing comprehensive program that has a goal of determining the Hubble constant to a systematic accuracy of 2%. As part of this program, we are currently obtaining 3.6 micron data using the Infrared Array Camera (IRAC) on Spitzer, and the program is designed to include JWST in the future. We demonstrate that the mid-infrared period-luminosity relation for Cepheids at 3.6 microns is the most accurate means of measuring Cepheid distances to date. At 3.6 microns, it is possible to minimize the known remaining systematic uncertainties in the Cepheid extragalactic distance scale. We discuss the advantages of 3.6 micron observations in minimizing systematic effects in the Cepheid calibration of the Hubble constant including the absolute zero point, extinction corrections, and the effects of metallicity on the colors and magnitudes of Cepheids. We are undertaking three independent tests of the sensitivity of the mid-IR Cepheid Leavitt Law to metallicity, which when combined will allow a robust constraint on the effect. Finally, we are providing a new mid-IR Tully-Fisher relation for spiral galaxies.

  6. Precision Distances with the Tip of the Red Giant Branch Method

    NASA Astrophysics Data System (ADS)

    Beaton, Rachael Lynn; Carnegie-Chicago Hubble Program Team

    2018-01-01

    The Carnegie-Chicago Hubble Program aims to construct a distance ladder that utilizes old stellar populations in the outskirts of galaxies to produce a high precision measurement of the Hubble Constant that is independent of Cepheids. The CCHP uses the tip of the red giant branch (TRGB) method, which is a statistical measurement technique that utilizes the termination of the red giant branch. Two innovations combine to make the TRGB a competitive route to the Hubble Constant (i) the large-scale measurement of trigonometric parallax by the Gaia mission and (ii) the development of both precise and accurate means of determining the TRGB in both nearby (~1 Mpc) and distant (~20 Mpc) galaxies. Here I will summarize our progress in developing these standardized techniques, focusing on both our edge-detection algorithm and our field selection strategy. Using these methods, the CCHP has determined equally precise (~2%) distances to galaxies in the Local Group (< 1 Mpc) and across the Local Volume (< 20 Mpc). The TRGB is, thus, an incredibly powerful and straightforward means to determine distances to galaxies of any Hubble Type and, thus, has enormous potential for putting any number of astrophyiscal phenomena on absolute units.

  7. The Carnegie Hubble Program: The Infrared Leavitt Law in IC 1613

    NASA Technical Reports Server (NTRS)

    Scowcroft, Victoria; Freedman, Wendy L.; Madore, Barry F.; Monson, Andrew J.; Persson, S. E.; Seibert, Mark; Rigby, Jane R.; Melbourne, Jason

    2013-01-01

    We have observed the dwarf galaxy IC 1613 at multiple epochs in the midinfrared using Spitzer and the in the near-infrared using the new FourStar near-IR camera on Magellan. We have constructed Cepheid period luminosity relations in the J, H, Ks, [3.6] and [4.5] bands and have used the run of their apparent distance moduli as a function of wavelength to derive the line of sight reddening and distance to IC 1613. Using a nineband fit, we find E(BV ) = 0.050.01 mag and an extinction corrected distance modulus of 0 = 24.29 0.03statistical 0.03systematic mag. By comparing our multiband and [3.6] distance moduli to results from the tip of the red giant branch and red clump distance indicators, we find that metallicity has no measurable effect on Cepheid distances at 3.6 m in the metallicity range 1.0 [Fe/H] 0.2, hence derivations of the Hubble constant at this wavelength require no correction for metallicity.

  8. A Perspective on Carnegie Corporation's Program, 1983-1997.

    ERIC Educational Resources Information Center

    Hamburg, David A.

    The Carnegie Corporation's mission is to continue Andrew Carnegie's philanthropic preoccupations with promoting education and world peace. In this essay, retiring Carnegie Corporation President David A. Hamburg provides a detailed accounting of his stewardship of the foundation since 1983, when he set forth new program directions in the context of…

  9. Improving Security in Software Acquisition and Runtime Integration With Data Retention Specifications

    DTIC Science & Technology

    2016-04-30

    Data Retention Specifications Daniel Smullen, Research Assistant, Carnegie Mellon University Travis Breaux, Assistant Professor, Carnegie Mellon... Carnegie Mellon University Travis Breaux, Assistant Professor, Carnegie Mellon University Cybersecurity Figure of Merit CAPT Brian Erickson, USN, SPAWAR...Integration With Data Retention Specifications Daniel Smullen—is a Research Assistant enrolled in the software engineering PhD program at Carnegie Mellon

  10. HUBBLE PROBES THE VIOLENT BIRTH OF STARS IN GALAXY NGC 253 [Left

    NASA Technical Reports Server (NTRS)

    2002-01-01

    An image of the spiral galaxy NGC 253, taken with a ground-based telescope. The galaxy is located about 8 million light-years away in the constellation Sculptor. Credit: Jay Gallagher (University of Wisconsin-Madison), Alan Watson (Lowell Observatory, Flagstaff, AZ), and NASA [Right] This NASA Hubble Space Telescope image of the core of the nearest starburst spiral galaxy, NGC 253, reveals violent star formation within a region 1,000 light-years across. A starburst galaxy has an exceptionally high rate of star birth, first identified by its excess of infrared radiation from warm dust. Hubble's high resolution allows astronomers to quantify complex structures in the starburst core of the galaxy for the first time, including luminous star clusters, dust lanes which trace regions of dense gas and filaments of glowing gas. Hubble identifies several regions of intense star formation, which include a bright, super-compact star cluster. These observations confirm that stars are often born in dense clusters within starbursts, and that dense gas coexists with and obscures the starburst core. This image was taken with Hubble's Wide Field Planetary Camera 2 (in PC mode). Credit: Carnegie Institution of Washington

  11. HUBBLE SPACE TELESCOPE ON TRACK FOR MEASURING THE EXPANSION RATE OF THE UNIVERSE

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Two international teams of astronomers, using NASA's Hubble Space Telescope, are reporting major progress in converging on an accurate measurement of the Universe's rate of expansion -- a value which has been debated for over half a century. These new results yield ranges for the age of the Universe from 9-12 billion years, and 11-14 billion years, respectively. The goal of the project is to measure the Hubble Constant to ten percent accuracy. The Hubble Space Telescope Key Project team, an international group of over 20 astronomers, is led by Wendy Freedman of Carnegie Observatories, Pasadena, CA, Robert Kennicutt, University of Arizona, Tucson, AZ, and Jeremy Mould, Mount Stromlo and Siding Springs Observatory, Australia. The group's interim results, announced at a meeting held at the Space Telescope Science Institute (STScI) in Baltimore, Maryland, are consistent with their preliminary result, announced in 1994, of 80 kilometers per second per megaparsec (km/sec/Mpc), based on observations of a galaxy in the Virgo cluster. 'We have five different ways of measuring the Hubble Constant with HST,' said Dr. Freedman. 'The results are coming in between 68 and 78 km/sec/Mpc.' (For example, at an expansion rate of 75 km/sec/Mpc, galaxies appear to be receding from us at a rate of 162,000 miles per hour for every 3.26 million light-years farther out we look). Two months ago, a second team, led by Allan Sandage, also of the Carnegie Observatories, Abhijit Saha, STScI, Gustav Tammann and Lukas Labhardt, Astronomical Institute, University of Basel, Duccio Macchetto and Nino Panagia, STScI/European Space Agency, reported a slower expansion rate of 57 km/sec/Mpc. The value of the Hubble Constant allows astronomers to calculate the expansion age of the Universe, the time elapsed since the Big Bang. Astronomers have been arguing recently whether the time since the Big Bang is consistent with the ages of the oldest stars. The ages are calculated from combining the expansion rate with an estimate of how much matter is in space. The younger age values from each team assume the Universe is at a critical density where it contains just enough matter to expand indefinitely. The higher age estimates are calculated based on a low density of matter in space. (See 'Science Background' for more information on the expanding Universe.) 'A point of great interest is whether the age of the Universe arrived at this way is really older than the independently derived ages of the oldest stars,' said Saha, an investigator on both Hubble teams. 'The numbers lean on the side that the stellar ages are a little lower, or that the hypothesis that we live in a critical density universe needs to be questioned,' said Saha. 'As further results accumulate over the next few years, we hope to tighten the constraints on these issues.' THE OBSERVATIONS The Key Project team is midway along in their three-year program to derive the expansion rate of the Universe based on precise distance measurements to galaxies. They have now measured Cepheid distances to a dozen galaxies, and are about halfway through their overall program. The Key Project team also presented a preliminary estimate of the distance to the Fornax cluster of galaxies. The estimate was obtained through the detection and measurement with the Hubble Space Telescope of pulsating stars known as Cepheid variables found in the Fornax cluster. The Fornax cluster is measured to be approximately as far away as the Virgo cluster of galaxies -- about 60 million light-years. The Key Project team member who led this effort, Caltech astronomer Barry Madore said, 'This cluster allows us to make independent estimates of the expansion rate of the Universe using a number of different techniques. All of these methods are now in excellent agreement. With Fornax we are now at turning point in this field.' The team is measuring Cepheid distances to the Virgo and Fornax clusters of galaxies as a complementary test. Their strategy is to compare and contrast expansion numbers from a variety of distance indicators. The Key Project team is systematically looking into a variety of methods for measuring distances. They are using Cepheids in a large sample to tie into five or six 'secondary methods'. One such secondary method relates the total luminosity of a galaxy to the rate at which the galaxy is spinning, the Tully-Fisher relation. Another secondary method makes use of a special class of exploding star known as a type Ia supernova. This phase of the Hubble Constant research will be completed within another two years. In contrast, the Sandage team focused on a single secondary distance indicator, one of the same indicators also used by the Key Project team, the type Ia supernova. Sandage maintains that these stars are 'standard bombs' according to theory. He suggests that when they explode they all reach exactly the same intrinsic brightness. This would make them extremely reliable 'standard candles,' (objects with a well-known intrinsic brightness) visible 1,000 times farther away than Cepheids. Since they are intrinsically brighter than any other standard candle, they offer the opportunity for an accurate measurement of the Universe's overall expansion by looking out the farthest. Although both teams are still in disagreement over the precise rate at which the Universe is expanding and on how old it is, they are optimistic that their estimates will continue to converge with further observations and analysis. * * * * Members of the Key Project team include W. Freedman (Carnegie Observatories), R. Kennicutt (University of Arizona), J. Mould (Mount Stromlo and Siding Springs Observatories, Australia), L. Ferrarese (Johns Hopkins University), H. Ford (Johns Hopkins University), J. Graham (Department of Terrestrial Magnetism), M. Han (University of Wisconsin), P. Harding (University of Arizona), J. Hoessel (University of Wisconsin), J. Huchra (Smithsonian/Harvard University), S. Hughes (Royal Greenwich Observatory, Cambridge), G. Illingworth (University of California, Santa Cruz), B.F. Madore (IPAC/Caltech), R. Phelps (Carnegie Observatories), A. Saha (Space Telescope Science Institute), N. Silbermann (IPAC), P. Stetson (Dominion Astrophysical Observatory), and S. Sakai (IPAC). Members of the Sandage team include A. Sandage (Carnegie Observatories), A. Saha (Space Telescope Science Institute), G.A. Tammann, and L. Labhardt (Astronomical Institute, University of Basel), F.D. Macchetto and N. Panagia (Space Telescope Science Institute/European Space Agency).

  12. The Evolution of an Adolescent Literacy Program: A Foundation's Journey

    ERIC Educational Resources Information Center

    Henriquez, Andres

    2005-01-01

    The Carnegie Corporation of New York is associated with the very foundations of literacy going back to the philanthropy of Andrew Carnegie himself and of the Corporation in its early years. Andrew Carnegie's legacy includes over 2,500 free public libraries that he saw as a link "bridging ignorance and education." In fact, Carnegie, the…

  13. Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant

    NASA Technical Reports Server (NTRS)

    Freedman, Wendy L.; Madore, Barry F.; Scowcroft, Victoria; Burns, Chris; Monson, Andy; Persson, S. Eric; Seibert, Mark; Rigby, Jane

    2012-01-01

    Using a mid-infrared calibration of the Cepheid distance scale based on recent observations at 3.6 micrometers with the Spitzer Space Telescope, we have obtained a new, high-accuracy calibration of the Hubble constant. We have established the mid-IR zero point of the Leavitt law (the Cepheid period-luminosity relation) using time-averaged 3.6 micrometers data for 10 high-metallicity, MilkyWay Cepheids having independently measured trigonometric parallaxes. We have adopted the slope of the PL relation using time-averaged 3.6micrometers data for 80 long-period Large Magellanic Cloud (LMC) Cepheids falling in the period range 0.8 < log(P) < 1.8.We find a new reddening-corrected distance to the LMC of 18.477 +/- 0.033 (systematic) mag. We re-examine the systematic uncertainties in H(sub 0), also taking into account new data over the past decade. In combination with the new Spitzer calibration, the systematic uncertainty in H(sub 0) over that obtained by the Hubble Space Telescope Key Project has decreased by over a factor of three. Applying the Spitzer calibration to the Key Project sample, we find a value of H(sub 0) = 74.3 with a systematic uncertainty of +/-2.1 (systematic) kilometers per second Mpc(sup -1), corresponding to a 2.8% systematic uncertainty in the Hubble constant. This result, in combination with WMAP7measurements of the cosmic microwave background anisotropies and assuming a flat universe, yields a value of the equation of state for dark energy, w(sub 0) = -1.09 +/- 0.10. Alternatively, relaxing the constraints on flatness and the numbers of relativistic species, and combining our results with those of WMAP7, Type Ia supernovae and baryon acoustic oscillations yield w(sub 0) = -1.08 +/- 0.10 and a value of N(sub eff) = 4.13 +/- 0.67, mildly consistent with the existence of a fourth neutrino species.

  14. The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-Infrared Observations of Cepheids

    NASA Technical Reports Server (NTRS)

    Scowcroft, Victoria; Freedman, Wendy L.; Madore, Barry F.; Monson, Andy; Persson, S. E.; Rich, Jeff; Seibert, Mark; Rigby, Jane R.

    2016-01-01

    Using Spitzer observations of classical Cepheids we have measured the true average distance modulus of the Small Magellanic Cloud (SMC) to be18.96 +/- 0.01 stat +/- 0.03sys mag (corresponding to 62+/- 0.3kpc), which is 0.48 +/- 0.01 mag more distant than the LMC. This is in agreement with previous results from Cepheid observations, as well as with measurements from other indicators such as RR Lyrae stars and the tip of the red giant branch. Utilizing the properties of the mid-infrared Leavitt Law we measured precise distances to individual Cepheids in the SMC, and have confirmed that the galaxy is tilted and elongated such that its eastern side is up to20 kpc closer than its western side. This is in agreement with the results from red clump stars and dynamical simulations of the Magellanic Clouds and Stream.

  15. Carnegie Learning Curricula and Cognitive Tutor™. What Works Clearinghouse Intervention Report

    ERIC Educational Resources Information Center

    What Works Clearinghouse, 2013

    2013-01-01

    "Carnegie Learning Curricula and Cognitive Tutor"®, published by Carnegie Learning, is a secondary math curricula that offers textbooks and interactive software to provide individualized, self-paced instruction based on student needs. The program includes pre-Algebra, Algebra I, Algebra II, and Geometry, as well as a three-course series…

  16. Faculty-Exchange Programs Promoting Change: Motivations, Experiences, and Influence of Participants in the Carnegie Mellon University-Portugal Faculty Exchange Program

    ERIC Educational Resources Information Center

    Patrício, Maria Teresa; Santos, Patrícia; Loureiro, Paulo Maia; Horta, Hugo

    2018-01-01

    The international mobility of faculty is increasing worldwide. Although studies have considered the experiences of academics abroad, less is known about faculty-exchange programs with policy objectives. This study helps to fill this gap by analyzing a nationwide structured faculty exchange program established by Carnegie Mellon University and…

  17. Carnegie Corporation of New York: Annual Report 1977 for the Fiscal Year Ended September 30.

    ERIC Educational Resources Information Center

    Carnegie Corp. of New York, NY.

    Carnegie Corporation of New York is a philanthropic foundation created by Andrew Carnegie in 1911 for the advancement and diffusion of knowledge and understanding. It is primarliy interested in education and in certain aspects of governmental affairs. Grants for specific programs are made to colleges and universities, professional associations,…

  18. Brandeis Science Posse: Talented Students Bring Diversity to the Field. Carnegie Results

    ERIC Educational Resources Information Center

    Theroux, Karen

    2013-01-01

    The Science Posse program at Brandeis University aims to increase the recruitment and retention of students from disadvantaged and underrepresented backgrounds in STEM (science, technology, engineering and mathematics) disciplines. A grant from Carnegie Corporation helped support the development of the program, which has brought 50 students from…

  19. Mathematics Intervention Utilizing Carnegie Learning's Cognitive Tutor® and Compass Learning's Odyssey Math®

    ERIC Educational Resources Information Center

    Barton, James M.

    2016-01-01

    Carnegie Learning's Cognitive Tutor®The purpose of this study is to determine whether there is a statistically significant difference between pre-test and post-test achievement scores when Compass Learning's Odyssey Math® is used together with Carnegie Learning's Math Cognitive Tutor® in a mathematics intervention program at ABC Middle School. The…

  20. A Hubble Diagram from Type II Supernovae Based Solely on Photometry: The Photometric Color Method

    NASA Astrophysics Data System (ADS)

    de Jaeger, T.; González-Gaitán, S.; Anderson, J. P.; Galbany, L.; Hamuy, M.; Phillips, M. M.; Stritzinger, M. D.; Gutiérrez, C. P.; Bolt, L.; Burns, C. R.; Campillay, A.; Castellón, S.; Contreras, C.; Folatelli, G.; Freedman, W. L.; Hsiao, E. Y.; Krisciunas, K.; Krzeminski, W.; Kuncarayakti, H.; Morrell, N.; Olivares E., F.; Persson, S. E.; Suntzeff, N.

    2015-12-01

    We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V - i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our golden sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data. This paper includes data gathered with the 6.5 m Magellan Telescopes, with the du Pont and Swope telescopes located at Las Campanas Observatory, Chile, and the Gemini Observatory, Cerro Pachon, Chile (Gemini Program GS-2008B-Q-56). Based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere, Chile (ESO Programmes 076.A-0156,078.D-0048, 080.A-0516, and 082.A-0526).

  1. 76 FR 72002 - National Register of Historic Places; Notification of Pending Nominations and Related Actions

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-11-21

    .../National Historic Landmarks Program. CALIFORNIA Alameda County Livermore Carnegie Library and Park, (California Carnegie Libraries MPS) 2155 3rd St., Livermore, 11000876 COLORADO Routt County Steamboat...

  2. The Carnegie-Irvine Galaxy Survey. V. Statistical Study of Bars and Buckled Bars

    NASA Astrophysics Data System (ADS)

    Li, Zhao-Yu; Ho, Luis C.; Barth, Aaron J.

    2017-08-01

    Simulations have shown that bars are subject to a vertical buckling instability that transforms thin bars into boxy or peanut-shaped structures, but the physical conditions necessary for buckling to occur are not fully understood. We use the large sample of local disk galaxies in the Carnegie-Irvine Galaxy Survey to examine the incidence of bars and buckled bars across the Hubble sequence. Depending on the disk inclination angle (I), a buckled bar reveals itself as either a boxy/peanut-shaped bulge (at high I) or as a barlens structure (at low I). We visually identify bars, boxy/peanut-shaped bulges, and barlenses, and examine the dependence of bar and buckled bar fractions on host galaxy properties, including Hubble type, stellar mass, color, and gas mass fraction. We find that the barred and unbarred disks show similar distributions in these physical parameters. The bar fraction is higher (70%-80%) in late-type disks with low stellar mass (M * < 1010.5 M ⊙) and high gas mass ratio. In contrast, the buckled bar fraction increases to 80% toward massive and early-type disks (M * > 1010.5 M ⊙), and decreases with higher gas mass ratio. These results suggest that bars are more difficult to grow in massive disks that are dynamically hotter than low-mass disks. However, once a bar forms, it can easily buckle in the massive disks, where a deeper potential can sustain the vertical resonant orbits. We also find a probable buckling bar candidate (ESO 506-G004) that could provide further clues to understand the timescale of the buckling process.

  3. A Family of SCAMPI Appraisal Methods

    DTIC Science & Technology

    2003-01-01

    CarnegieMellon Software Engineering Institute A Family of SCAMPISM Appraisal Methods Will Hayes Gene Miluk Dave Kitson Report Documentation Page Form...COVERED 00-00-2003 to 00-00-2003 4. TITLE AND SUBTITLE A Family of SCAMPIsm Appraisal Methods 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM...Based Management © 2003 by Carnegie Mellon University wh SEPG03 page 17 CarnegieMellon Software Engineering Institute Presentation Outline Examples of

  4. Benefits of CMM-Based Software Process Improvement: Initial Results

    DTIC Science & Technology

    1994-08-01

    Institute Carnegie Mellon University Pittsburgh, Pennsylvania 15213 This report was prepar the SEI Joint Program Office HQ ESC/ENS 5 Eglin Street Hanscom AFB...Miller, Lt Col, USAF SEI Joint Program Office This work is sponsored by the U.S. Department of Defense. Copyright 0 1994 by Carnegie Mellon University...categories: descriptive information about the organizations, information about their process improvement and measurement programs , and data about the

  5. The Carnegie-Irvine Galaxy Survey. V. Statistical Study of Bars and Buckled Bars

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Li, Zhao-Yu; Ho, Luis C.; Barth, Aaron J., E-mail: lizy@shao.ac.cn

    Simulations have shown that bars are subject to a vertical buckling instability that transforms thin bars into boxy or peanut-shaped structures, but the physical conditions necessary for buckling to occur are not fully understood. We use the large sample of local disk galaxies in the Carnegie-Irvine Galaxy Survey to examine the incidence of bars and buckled bars across the Hubble sequence. Depending on the disk inclination angle ( i ), a buckled bar reveals itself as either a boxy/peanut-shaped bulge (at high i ) or as a barlens structure (at low i ). We visually identify bars, boxy/peanut-shaped bulges, andmore » barlenses, and examine the dependence of bar and buckled bar fractions on host galaxy properties, including Hubble type, stellar mass, color, and gas mass fraction. We find that the barred and unbarred disks show similar distributions in these physical parameters. The bar fraction is higher (70%–80%) in late-type disks with low stellar mass ( M {sub *} < 10{sup 10.5} M {sub ⊙}) and high gas mass ratio. In contrast, the buckled bar fraction increases to 80% toward massive and early-type disks ( M {sub *} > 10{sup 10.5} M {sub ⊙}), and decreases with higher gas mass ratio. These results suggest that bars are more difficult to grow in massive disks that are dynamically hotter than low-mass disks. However, once a bar forms, it can easily buckle in the massive disks, where a deeper potential can sustain the vertical resonant orbits. We also find a probable buckling bar candidate (ESO 506−G004) that could provide further clues to understand the timescale of the buckling process.« less

  6. FAR-FLUNG GALAXY CLUSTERS MAY REVEAL FATE OF UNIVERSE

    NASA Technical Reports Server (NTRS)

    2002-01-01

    A selection of NASA Hubble Space Telescope snapshots of huge galaxy clusters that lie far away and far back in time. These are selected from a catalog of 92 new clusters uncovered during a six-year Hubble observing program known as the Medium Deep Survey. If the distances and masses of the clusters are confirmed by ground based telescopes, the survey may hold clues to how galaxies quickly formed into massive large-scale structures after the big bang, and what that may mean for the eventual fate of the expanding universe. The images are each a combination of two exposures in yellow and deep red taken with Hubble's Wide Field and Planetary Camera 2. Each cluster's distance is inferred from the reddening of the starlight, which is due to the expansion of space. Astronomers assume these clusters all formed early in the history of the universe. HST133617-00529 (left) This collection of spiral and elliptical galaxies lies an estimated 4 to 6 billion light-years away. It is in the constellation of Virgo not far from the 3rd magnitude star Zeta Virginis. The brighter galaxies in this cluster have red magnitudes between 20 and 22 near the limit of the Palomar Sky Survey. The bright blue galaxy (upper left) is probably a foreground galaxy, and not a cluster member. The larger of the galaxies in the cluster are probably about the size of our Milky Way Galaxy. The diagonal line at lower right is an artificial satellite trail. HST002013+28366 (upper right) This cluster of galaxies lies in the constellation of Andromeda a few degrees from the star Alpheratz in the northeast corner of the constellation Pegasus. It is at an estimated distance of 4 billion light-years, which means the light we are seeing from the cluster is as it appeared when the universe was roughly 2/3 of its present age. HST035528+09435 (lower right) At an estimated distance of about 7 to 10 billion light-years (z=1), this is one of the farthest clusters in the Hubble sample. The cluster lies in the constellation of Taurus. Credit: K. Ratnatunga, R. Griffiths (Carnegie Mellon University); and NASA

  7. Carnegie Foundation Creates New "Owner's Manual" for Doctoral Programs

    ERIC Educational Resources Information Center

    Wasley, Paula

    2007-01-01

    In his 1990 book "Scholarship Reconsidered: Priorities of the Professoriate", Ernest L. Boyer, who was then president of the Carnegie Foundation for the Advancement of Teaching, analyzed the balance between teaching and research in the scholarly endeavors of that era. His conclusion that the university rewarded research at the expense of teaching…

  8. Excellence: An Immodest Proposal. Carnegie Perspectives

    ERIC Educational Resources Information Center

    Shulman, Lee S.

    2005-01-01

    The writer describes a site visit to the teaching hospital of a major American medical school, part of the Carnegie Foundation's ten-year program of research on how lawyers, engineers, clergy, school teachers, nurses, and physicians are taught and how they learn. Of particular note to Schulman was an exercise known as "M&M" (Morbidity and…

  9. A Type II Supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS Surveys

    NASA Astrophysics Data System (ADS)

    de Jaeger, T.; González-Gaitán, S.; Hamuy, M.; Galbany, L.; Anderson, J. P.; Phillips, M. M.; Stritzinger, M. D.; Carlberg, R. G.; Sullivan, M.; Gutiérrez, C. P.; Hook, I. M.; Howell, D. Andrew; Hsiao, E. Y.; Kuncarayakti, H.; Ruhlmann-Kleider, V.; Folatelli, G.; Pritchet, C.; Basa, S.

    2017-02-01

    The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35 mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27 mag, I.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universe’s matter density: {{{Ω }}}m={0.32}-0.21+0.30 providing a new independent evidence for dark energy at the level of two sigma. This paper includes data gathered with the 6.5 m Magellan Telescopes, with the du Pont and Swope telescopes located at Las Campanas Observatory, Chile; and the Gemini Observatory, Cerro Pachon, Chile (Gemini Program N-2005A-Q-11, GN-2005B-Q-7, GN-2006A-Q-7, GS-2005A-Q-11, GS-2005B-Q-6, and GS-2008B-Q-56). Based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere, Chile (ESO Programmes 076.A-0156,078.D-0048, 080.A-0516, and 082.A-0526).

  10. LIFTING THE VEIL OF DUST TO REVEAL THE SECRETS OF SPIRAL GALAXIES

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Astronomers have combined information from the NASA Hubble Space Telescope's visible- and infrared-light cameras to show the hearts of four spiral galaxies peppered with ancient populations of stars. The top row of pictures, taken by a ground-based telescope, represents complete views of each galaxy. The blue boxes outline the regions observed by the Hubble telescope. The bottom row represents composite pictures from Hubble's visible- and infrared-light cameras, the Wide Field and Planetary Camera 2 (WFPC2) and the Near Infrared Camera and Multi-Object Spectrometer (NICMOS). Astronomers combined views from both cameras to obtain the true ages of the stars surrounding each galaxy's bulge. The Hubble telescope's sharper resolution allows astronomers to study the intricate structure of a galaxy's core. The galaxies are ordered by the size of their bulges. NGC 5838, an 'S0' galaxy, is dominated by a large bulge and has no visible spiral arms; NGC 7537, an 'Sbc' galaxy, has a small bulge and loosely wound spiral arms. Astronomers think that the structure of NGC 7537 is very similar to our Milky Way. The galaxy images are composites made from WFPC2 images taken with blue (4445 Angstroms) and red (8269 Angstroms) filters, and NICMOS images taken in the infrared (16,000 Angstroms). They were taken in June, July, and August of 1997. Credits for the ground-based images: Allan Sandage (The Observatories of the Carnegie Institution of Washington) and John Bedke (Computer Sciences Corporation and the Space Telescope Science Institute) Credits for WFPC2 and NICMOS composites: NASA, ESA, and Reynier Peletier (University of Nottingham, United Kingdom)

  11. HUBBLE'S TOP TEN GRAVITATIONAL LENSES

    NASA Technical Reports Server (NTRS)

    2002-01-01

    The NASA Hubble Space Telescope serendipitous survey of the sky has uncovered exotic patterns, rings, arcs and crosses that are all optical mirages produced by a gravitational lens, nature's equivalent of having giant magnifying glass in space. Shown are the top 10 lens candidates uncovered in the deepest 100 Hubble fields. Hubble's sensitivity and high resolution allow it to see faint and distant lenses that cannot be detected with ground-based telescopes whose images are blurred by Earth's atmosphere. [Top Left] - HST 01248+0351 is a lensed pair on either side of the edge-on disk lensing galaxy. [Top Center] - HST 01247+0352 is another pair of bluer lensed source images around the red spherical elliptical lensing galaxy. Two much fainter images can be seen near the detection limit which might make this a quadruple system. [Top Right] - HST 15433+5352 is a very good lens candidate with a bluer lensed source in the form of an extended arc about the redder elliptical lensing galaxy. [Middle Far Left] - HST 16302+8230 could be an 'Einstein ring' and the most intriguing lens candidate. It has been nicknamed the 'the London Underground' since it resembles that logo. [Middle Near Left] - HST 14176+5226 is the first, and brightest lens system discovered in 1995 with the Hubble telescope. This lens candidate has now been confirmed spectroscopically using large ground-based telescopes. The elliptical lensing galaxy is located 7 billion light-years away, and the lensed quasar is about 11 billion light-years distant. [Middle Near Right] - HST 12531-2914 is the second quadruple lens candidate discovered with Hubble. It is similar to the first, but appears smaller and fainter. [Middle Far Right] - HST 14164+5215 is a pair of bluish lensed images symmetrically placed around a brighter, redder galaxy. [Bottom Left] - HST 16309+8230 is an edge-on disk-like galaxy (blue arc) which has been significantly distorted by the redder lensing elliptical galaxy. [Bottom Center] - HST 12368+6212 is a blue arc in the Hubble Deep Field (HDF). [Bottom Right] - HST 18078+4600 is a blue arc caused by the gravitational potential of a small group of 4 galaxies. Credit: Kavan Ratnatunga (Carnegie Mellon Univ.) and NASA

  12. A HUBBLE DIAGRAM FROM TYPE II SUPERNOVAE BASED SOLELY ON PHOTOMETRY: THE PHOTOMETRIC COLOR METHOD

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    De Jaeger, T.; González-Gaitán, S.; Galbany, L.

    2015-12-20

    We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V − i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our goldenmore » sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data.« less

  13. Federal Reorganization: Education and Scholarship. A Report of the Carnegie Council on Policy Studies in Higher Education.

    ERIC Educational Resources Information Center

    Carnegie Council on Policy Studies in Higher Education, Berkeley, CA.

    The federal government is approaching a new round of consideration of administrative reorganization, including the areas of education and of support for scholarly endeavors. The concern of the Carnegie Council is that the government, in view of its recent experience with rapid program expansion and of the vast problems ahead in health care and…

  14. Carnegie Mellon University's MMM program: management education for 21st-century physicians.

    PubMed

    Korevaar, W C; Pearson, R W

    2001-01-01

    The number and types of executive and graduate-level management programs for physicians have exploded in recent years. These programs take on a variety of formats, ranging from executive seminars to master's-level degree programs. Options for physicians obtaining the master's degree tend to be either regionally based programs in traditional evening classes or nationally based programs that combine executive education formats with distance education. This paper examines a nationally based program - the Master of Medical Management (MMM) - from the perspectives of an administrator and a graduate of the program. It offers reasons for the growth of similar programs and data from students enrolled in the Carnegie Mellon University MMM program. The paper also examines educational outcomes in the form of behavioral competencies that the physicians acquired in the program. It concludes with reflections on the future of the MMM and related programs for physician executives in the 21st century.

  15. The Evolution of a Graduate Writing Program: The Master of Arts in Professional Writing at Carnegie Mellon University. CDC Technical Report No. 33.

    ERIC Educational Resources Information Center

    Jones, G. H.; Steinberg, E. R.

    The Master of Arts in Professional Writing (MAPW) offered by Carnegie Mellon University (Pennsylvania) is designed for students who want careers as document designers in industry and government, where they will plan, write, and evaluate computer manuals and on-line documentation, training and instructional materials, technical reports, and a wide…

  16. Software Architecture for Big Data Systems

    DTIC Science & Technology

    2014-03-27

    Software Architecture: Trends and New Directions #SEIswArch © 2014 Carnegie Mellon University Software Architecture for Big Data Systems...AND SUBTITLE Software Architecture for Big Data Systems 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT...ih - . Software Architecture: Trends and New Directions #SEIswArch © 2014 Carnegie Mellon University WHAT IS BIG DATA ? FROM A SOFTWARE

  17. Integrating a Natural Language Message Pre-Processor with UIMA

    DTIC Science & Technology

    2008-01-01

    Carnegie Mellon Language Technologies Institute NL Message Preprocessing with UIMA Copyright © 2008, Carnegie Mellon. All Rights Reserved...Integrating a Natural Language Message Pre-Processor with UIMA Eric Nyberg, Eric Riebling, Richard C. Wang & Robert Frederking Language Technologies Institute...with UIMA 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT NUMBER 5e. TASK NUMBER 5f. WORK UNIT NUMBER

  18. The Carnegie Chicago Hubble Program: The Mid-Infrared Colours of Cepheids and the Effect of Metallicity on the CO Band-Head at 4.6 Micron

    NASA Technical Reports Server (NTRS)

    Scowcroft, Victoria; Seibert, Mark; Freedman, Wendy L.; Beaton, Rachael L.; Madore, Barry F.; Monson, Andrew J.; Rich, Jeffery A.; Rigby, Jane R.

    2016-01-01

    We compare mid-infrared (IR) 3.6 and 4.5 micron Warm Spitzer observations for Cepheids in the Milky Way and the Large and Small Magellanic Clouds. Using models, we explore in detail the effect of the CO rotation-vibration band-head at 4.6 micron on the mid-IR photometry. We confirm the temperature sensitivity of the CO band-head at 4.6 micron and find no evidence for an effect at 3.6 micron. We compare the ([3.6]-[4.5]) period-colour relations in the MW, LMC and SMC. The slopes of the period-colour relations for the three galaxies are in good agreement, but there is a trend in zero-point with metallicity, with the lowest metallicity Cepheids having redder mid-IR colours. Finally, we present a colour-[Fe/H] relation based on published spectroscopic metallicities. This empirical relation, calibrated to the metallicity system of Genovali et al., demonstrates that the ([3.6]-[4.5]) colour provides a reliable metallicity indicator for Cepheids, with a precision comparable to current spectroscopic determinations.

  19. Not your grandfather's concert hall

    NASA Astrophysics Data System (ADS)

    Cooper, Russell; Malenka, Richard; Griffith, Charles; Friedlander, Steven

    2004-05-01

    The opening of Judy and Arthur Zankel Hall on 12 September 2003, restores Andrew Carnegie's original 1891 concept of having three outstanding auditoriums of different sizes under one roof, and creates a 21st-century venue for music performance and education. With concerts ranging from early music to avant-garde multimedia productions, from jazz to world music, and from solo recitals to chamber music, Zankel Hall expands the breadth and depth of Carnegie Hall's offerings. It allows for the integration of programming across three halls with minifestivals tailored both to the size and strengths of each hall and to the artists and music to be performed. The new flexible space also provides Carnegie Hall with an education center equipped with advanced communications technology. This paper discusses the unique program planned for this facility and how the architects, theatre consultants, and acousticians developed a design that fulfilled the client's expectations and coordinated the construction of the facility under the floor of the main Isaac Stern Auditorium without having to cancel a single performance.

  20. Hubble Uncovers Evidence of Farthest Planet Forming From its Star

    NASA Image and Video Library

    2017-12-08

    Astronomers using NASA's Hubble Space Telescope have found compelling evidence of a planet forming 7.5 billion miles away from its star, a finding that may challenge current theories about planet formation. Of the almost 900 planets outside our solar system that have been confirmed to date, this is the first to be found at such a great distance from its star. The suspected planet is orbiting the diminutive red dwarf TW Hydrae, a popular astronomy target located 176 light-years away from Earth in the constellation Hydra the Sea Serpent. Read more: 1.usa.gov/196B6lZ NASA, ESA, J. Debes (STScI), H. Jang-Condell (University of Wyoming), A. Weinberger (Carnegie Institution of Washington), A. Roberge (Goddard Space Flight Center), G. Schneider (University of Arizona/Steward Observatory), and A. Feild (STScI/AURA) NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram

  1. Establishing The Pasadena Seismological Laboratory: An Adventure in Scientific Collaboration

    NASA Astrophysics Data System (ADS)

    Hazen, M. H.

    2002-05-01

    The 1906 San Francisco earthquake jolted Berkeley geologist Harry O. Wood (1879-1958) into a lifetime of seismological research that included the establishment of a seismic monitoring network in southern California, the co-invention of a seismograph capable of measuring short-period earthquakes, and the implementation of a public-safety campaign. None of these initiatives would have been possible without the support of the Carnegie Institution, a Washington DC-based research organization that supported not only exceptional individuals (as founder Andrew Carnegie had stipulated), but also large-scale, collaborative investigations. Wood published his plan for a "western United States" earthquake research program in 1916, but it was not until he moved to Washington during World War I that he made contacts that transformed his dream into a reality. While working at the National Research Council, Wood shared his vision with astronomer George Ellery Hale, geologist Arthur L. Day and, finally, Carnegie president John C. Merriam. Merriam was a Californian, a geologist, and a strong proponent of collaborative science. In 1921, the Carnegie Advisory Committee on Seismology - the first organization "of this magnitude" in American research - was formed. Initially, the program operated from an office at the Mount Wilson Observatory, where Wood was in charge of the daily operations. Then, in 1926, a joint venture with the California Institute of Technology was launched. Located in the mountains west of Pasadena, the Seismological Laboratory coordinated a range of scientific efforts. By 1930, thirteen American cities had Wood-Anderson seismographs in place, quantities of data had been acquired, new fault zones had been identified, and Beno Gutenberg and Charles F. Richter had been attracted to the program. Over the years, the U.S. Coast and Geodetic Survey and other government agencies also contributed to the effort. In the mid-1930s, the Carnegie Institution transferred the program to Caltech, but the Institution did not abandon seismology. Today, individual scientists like Harry Wood continue to shape the Institution's research agenda. And, like Gutenberg, they attempt to relate movements deep within the earth to the shaping of the earth's crust.

  2. The BBN (Bolt Beranek and Newman) Knowledge Acquisition Project. Phase 1. Functional Description; Test Plan.

    DTIC Science & Technology

    1987-05-01

    Computers . " Symbolics. Inc. 8. Carnegie Group. Inc KnoiledgeCraft Carnegie Group, Inc.. 1985. .- 9. Moser, Margaret, An Overviev of NIKL. Section of BBN...ORGANIZATION NAME AND ADDRESS I0. PROGRAM ELEMENT. PROJECT. TASK BBN Laboratories Inc. AREAAWoRIUNTNUMER_ 10 Moulton St. Cambridge, MA 02238 It...knowledge representation, expert systems; strategic computing , . A 20 ABSTRACT (Contnue an r rerse ide If neceaesary and Identify by block number) This

  3. A Closer Look at 804: A Summary of Considerations for DoD Program Managers

    DTIC Science & Technology

    2011-12-01

    aimed at changing the culture from one that is fo- cused typically on a single delivery to a new model that comprises multiple deliveries to es...under the Agency CIOs, and de - velop flexible budget models that align with modular development. • Launch an interactive platform for pre-RFP agency...permission@sei.cmu.edu. TM Carnegie Mellon Software Engineering Institute (stylized), Carnegie Mellon Software Engineering Institute (and de - sign), Simplex

  4. Focus on Resiliency: A Process-Oriented Approach to Security

    DTIC Science & Technology

    2005-11-01

    by ANSI Std Z39-18 © 2005 Carnegie Mellon University CSI v1.0 2 Agenda About the SEI Characterizing the problem Security, resiliency, and risk A...2005 Carnegie Mellon University CSI v1.0 5 SEI Technical Programs Product Line Systems Dynamic Systems Software Engineering Process Management...University CSI v1.0 7 What is the problem? Is your organization’s security capability sufficient to identify and manage risks that result from failed

  5. Pittsburgh Public School District / Carnegie Mellon University Robotics Team Participation in the US First Competition

    NASA Technical Reports Server (NTRS)

    Stroupe, Ashley

    2002-01-01

    FIRST, For Inspiration and Recognition of Science and Technology, is an international program designed to encourage junior and senior high school students to participate in science and technology related activities. FIRST attempts to increase enthusiasm for technology by providing a competitive environment in which to demonstrate robotics technology designed for a particular set of tasks. Carnegie Mellon University provided student members of the project the opportunity to complete the design, construction, testing, and operation of a robot. Electrical, mechanical, and programming skills were stressed, with both adult and senior students acting as mentors for more junior members. Teamwork and integration was also stressed in order to provide students with a realistic feel for project-based work. Finally, an emphasis was placed on recruiting students with greater difficulty in entering technological fields: girls and ethnic minorities and students leaning toward humanities (especially art). Carnegie Mellon built a relationship with Taylor Allderdice High School that lasted four years. For four years, the success of the project increased each year. Each term, the students successfully designed and built a working robot that could fully participate in the competition. The enthusiasm of the students has been the cornerstone of the recruit of new students, keeping the project growing and vital. Carnegie Mellon's participation with Allderdice has been an overall great success.

  6. SMART: Analyzing the Reuse Potential of Legacy Systems in Service- Oriented Architecture (SOA) Environments

    DTIC Science & Technology

    2009-04-09

    technical faculty for the Master in Software Engineering program at CMU. Grace holds a B.Sc. in Systems Engineering and an Executive MBA from Icesi...University in Cali, Colombia ; and a Master in Software Engineering from Carnegie Mellon University. 3 Version 1.7.3—SEI Webinar—April 2009 © 2009 Carnegie...Resources and Training SMART Report • http://www.sei.cmu.edu/publications/documents/08.reports/08tn008.html Public Courses • Migration of Legacy

  7. HUBBLE SPIES GLOBULAR CLUSTER IN NEIGHBORING GALAXY

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Hubble Space Telescope has captured a view of a globular cluster called G1, a large, bright ball of light in the center of the photograph consisting of at least 300,000 old stars. G1, also known as Mayall II, orbits the Andromeda galaxy (M31), the nearest major spiral galaxy to our Milky Way. Located 130,000 light-years from Andromeda's nucleus, G1 is the brightest globular cluster in the Local Group of galaxies. The Local Group consists of about 20 nearby galaxies, including the Milky Way. The crisp image is comparable to ground-based telescope views of similar clusters orbiting the Milky Way. The Andromeda cluster, however, is nearly 100 times farther away. A glimpse into the cluster's finer details allow astronomers to see its fainter helium-burning stars whose temperatures and brightnesses show that this cluster in Andromeda and the oldest Milky Way clusters have approximately the same age. These clusters probably were formed shortly after the beginning of the universe, providing astronomers with a record of the earliest era of galaxy formation. During the next two years, astronomers will use Hubble to study about 20 more globular clusters in Andromeda. The color picture was assembled from separate images taken in visible and near-infrared wavelengths taken in July of 1994. CREDIT: Michael Rich, Kenneth Mighell, and James D. Neill (Columbia University), and Wendy Freedman (Carnegie Observatories), and NASA Image files in GIF and JPEG format and captions may be accessed on Internet via anonymous ftp from oposite.stsci.edu in /pubinfo.

  8. Galaxy NGC 1512

    NASA Technical Reports Server (NTRS)

    1999-01-01

    A rainbow of colors is captured in the center of a magnificent barred spiral galaxy, as witnessed by the three cameras of NASA's Hubble Space Telescope.

    The color-composite image of the galaxy NGC 1512 was created from seven images taken with the JPL-designed and built Wide Field and Planetary Camera 2 (WFPC-2), along with the Faint Object Camera and the Near Infrared Camera and Multi-Object Spectrometer. Hubble's unique vantage point high above the atmosphere allows astronomers to see objects over a broad range of wavelengths from the ultraviolet to the infrared and to detect differences in the regions around newly born stars.

    The new image is online at http://oposite.stsci.edu/pubinfo/pr/2001/16 and http://www.jpl.nasa.gov/images/wfpc .

    The image reveals a stunning 2,400 light-year-wide circle of infant star clusters in the center of NGC 1512. Located 30 million light-years away in the southern constellation of Horologium, NGC 1512 is a neighbor of our Milky Way galaxy.

    With the Hubble data, a team of Israeli and American astronomers performed one of the broadest, most detailed studies ever of such star-forming regions. Results will appear in the June issue of the Astronomical Journal. The team includes Dr. Dan Maoz, Tel-Aviv University, Israel and Columbia University, New York, N.Y.; Dr. Aaron J. Barth, Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.; Dr. Luis C. Ho, The Observatories of the Carnegie Institution of Washington; Dr. Amiel Sternberg, Tel-Aviv University, Israel; and Dr. Alexei V. Filippenko, University of California, Berkeley.

    The Space Telescope Science Institute, Baltimore, Md., manages space operations for the Hubble Space Telescope for NASA's Office of Space Science, Washington, D.C. The Institute is operated by the Association of Universities for Research in Astronomy Inc., for NASA under contract with NASA's Goddard Space Flight Center, Greenbelt, Md. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. JPL is a division of the California Institute of Technology in Pasadena.

    Additional information about the Hubble Space Telescope is online at http://www.stsci.edu . More information about the Wide Field and Planetary Camera 2 is at http://wfpc2.jpl.nasa.gov.

  9. Study of the Careers of Participants in UMTA's Transit Management Programs (Section 10)

    DOT National Transportation Integrated Search

    1983-11-01

    This paper contains the results of a study of two Transit Management Training Programs for which UMTA provides fellowships. From 1969 to 1982, 428 fellowships were granted for attending a program at Carnegie-Mellon University, and 769 for attending N...

  10. Academic Library Development Program: A Self Study.

    ERIC Educational Resources Information Center

    Carnegie-Mellon Univ., Pittsburgh, PA. University Libraries.

    Results of a 4-month library self-evaluation program conducted by staff members at Carnegie-Mellon University Libraries are reported in this document. The study was conducted using the Academic Library Development Program (ALDP), a self-improvement strategy for libraries to evaluate and develop their performance. The study team consisting of four…

  11. Complexity and Safety (FAA)

    DTIC Science & Technology

    2016-10-27

    Software Engineering Institute Carnegie Mellon University Pittsburgh, PA 15213 © 2016 Carnegie Mellon University [DISTRIBUTION STATEMENT A: This... Carnegie Mellon University [DISTRIBUTION STATEMENT A: This material has been approved for public release and unlimited distribution] Copyright 2016 Carnegie ... Carnegie Mellon University for the operation of the Software Engineering Institute, a federally funded research and development center sponsored by

  12. Hubble Space Telescope: The GO and GTO Observing Programs. Version 1.0

    NASA Technical Reports Server (NTRS)

    Saha, Abhijit

    1990-01-01

    Selected information from the current Hubble Space Telescope (HST) science programs for the Guaranteed Time Observers (GTO's) and General Observers (GO's) is presented. Included are program abstracts, detailed listings of specific targets, and exposure information.

  13. Standardizing Type Ia supernovae optical brightness using near-infrared rebrightening time

    NASA Astrophysics Data System (ADS)

    Shariff, H.; Dhawan, S.; Jiao, X.; Leibundgut, B.; Trotta, R.; van Dyk, D. A.

    2016-12-01

    Accurate standardization of Type Ia supernovae (SNIa) is instrumental to the usage of SNIa as distance indicators. We analyse a homogeneous sample of 22 low-z SNIa, observed by the Carnegie Supernova Project in the optical and near-infrared (NIR). We study the time of the second peak in the J band, t2, as an alternative standardization parameter of SNIa peak optical brightness, as measured by the standard SALT2 parameter mB. We use BAHAMAS, a Bayesian hierarchical model for SNIa cosmology, to estimate the residual scatter in the Hubble diagram. We find that in the absence of a colour correction, t2 is a better standardization parameter compared to stretch: t2 has a 1σ posterior interval for the Hubble residual scatter of σΔμ = {0.250, 0.257} mag, compared to σΔμ = {0.280, 0.287} mag when stretch (x1) alone is used. We demonstrate that when employed together with a colour correction, t2 and stretch lead to similar residual scatter. Using colour, stretch and t2 jointly as standardization parameters does not result in any further reduction in scatter, suggesting that t2 carries redundant information with respect to stretch and colour. With a much larger SNIa NIR sample at higher redshift in the future, t2 could be a useful quantity to perform robustness checks of the standardization procedure.

  14. A New Twist on an Old Theme.

    ERIC Educational Resources Information Center

    Marchetti, Honey

    A work-study student assistant was employed at the Carnegie Mellon University Engineering and Science Library to help prepare documentation for a new library program. The student, a junior professional writing major, used the Apple Macintosh microcomputer to design a brochure, billing worksheet, and spreadsheet for the new program. On completion…

  15. 78 FR 14578 - Proposed Flood Hazard Determinations

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-03-06

    ... 15017. Borough of Carnegie Borough Building, 1 Glass Street, Carnegie, PA 15106. Borough of Castle... of Rosslyn Farms Rosslyn Farms Borough Secretary's Office, 421 Kings Highway, Carnegie, PA 15106... Office, 301 Lindsay Road, Carnegie, PA 15106. Township of Shaler Shaler Township Hall, 300 Wetzel Road...

  16. Joining Undergraduate Liberal Arts Colleges with a Graduate M.A.T. Program To Implement the Holmes and Carnegie Recommendations.

    ERIC Educational Resources Information Center

    Winter, Stephen S.

    This paper describes a combined B.A.-M.A.T. program, a project planned jointly by Kenyon College and Tufts University for the recruitment of outstanding liberal arts students who are interested in teaching careers. The program fulfills the requirements for teacher certification at the middle or secondary level in Massachusetts. The program offered…

  17. 78 FR 22285 - Notice of Inventory Completion: Carnegie Museum of Natural History, Pittsburgh, PA

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-04-15

    ....R50000] Notice of Inventory Completion: Carnegie Museum of Natural History, Pittsburgh, PA AGENCY: National Park Service, Interior. ACTION: Notice. SUMMARY: The Carnegie Museum of Natural History has... associated funerary objects should submit a written request to the Carnegie Museum of Natural History. If no...

  18. Quality Control Review of the PricewaterhouseCoopers LLP FY 2014 Single Audit of Carnegie Mellon University

    DTIC Science & Technology

    2015-12-17

    No. DODIG-2016-034 D E C E M B E R 1 7 , 2 0 1 5 Quality Control Review of the PricewaterhouseCoopers LLP FY 2014 Single Audit of Carnegie ...ALEXANDRIA, VIRGINIA 22350-1500 December 17, 2015 Audit Partner PricewaterhouseCoopers LLP Board of Trustees Carnegie Mellon University Director, Sponsored...Projects Accounting Carnegie Mellon University SUBJECT: Quality Control Review of the PricewaterhouseCoopers LLP FY 2014 Single Audit of Carnegie

  19. Just Care: Learning from and with Graduate Students in a Doctor of Nursing Practice Program

    ERIC Educational Resources Information Center

    Boquet, Elizabeth; Kazer, Meredith; Manister, Nancy; Lucas, Owen; Shaw, Michael; Madaffari, Valerie; Gannett, Cinthia

    2015-01-01

    In 2010, Fairfield University, a Jesuit Carnegie Masters Level 1 University located in the Northeast, established its first doctoral-level program: the Doctorate of Nursing Practice (DNP). In a developing program such as the DNP, some of the most pressing concerns of current rhetoric and writing in the disciplines align and interact with the…

  20. The Carnegie Initiative on the Doctorate: The Case of Mathematics. Carnegie Essays on the Doctorate: Mathematics.

    ERIC Educational Resources Information Center

    Bass, Hyman

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  1. Do Psychology Department Mission Statements Reflect the American Psychological Association Undergraduate Learning Goals?

    ERIC Educational Resources Information Center

    Warchal, Judith R.; Ruiz, Ana I.; You, Di

    2017-01-01

    This study focuses on the inclusion of the American Psychological Association's learning goals in the mission statements of undergraduate psychology programs across the US. We reviewed the mission statements available on websites for 1336 psychology programs listed in the Carnegie classification. Results of a content analysis revealed that of the…

  2. More than a Network: Building Professional Communities for Educational Improvement

    ERIC Educational Resources Information Center

    Dolle, Jonathan R.; Gomez, Louis M.; Russell, Jennifer Lin; Bryk, Anthony S.

    2013-01-01

    This chapter is a case study of the Carnegie Foundation for the Advancement of Teaching's Pathways [TM] program. The goal of the Statway [Registered Trademark] and Quantway [Registered Trademark] pathways is to improve the success rate of community college students who place into developmental mathematics. What makes these programs unique is…

  3. Through the Looking-Glass Portfolio: The Journey of Preservice Teachers in Becoming Reflective Practitioners.

    ERIC Educational Resources Information Center

    Peters, William H.

    To gain insights into preservice teachers' growing capacity to be exploring, reflective practitioners, portfolio assessment is being adopted in some teacher education programs. The teacher as reflective practitioner and portfolio assessment became the foundations of one Carnegie-I research university's four-phase secondary education program.…

  4. Fall 2014 SEI Research Review High Confidence Cyber Physical Systems

    DTIC Science & Technology

    2014-10-28

    2014 Carnegie Mellon University Fall 2014 SEI Research Review High Confidence Cyber Physical Systems Software Engineering Institute Carnegie... Research Review de Niz Oct 28th, 2014 © 2014 Carnegie Mellon University Copyright 2014 Carnegie Mellon University This material is based upon work...Software Engineering Institute, a federally funded research and development center. Any opinions, findings and conclusions or recommendations expressed

  5. COSMOS: Carnegie Observatories System for MultiObject Spectroscopy

    NASA Astrophysics Data System (ADS)

    Oemler, A.; Clardy, K.; Kelson, D.; Walth, G.; Villanueva, E.

    2017-05-01

    COSMOS (Carnegie Observatories System for MultiObject Spectroscopy) reduces multislit spectra obtained with the IMACS and LDSS3 spectrographs on the Magellan Telescopes. It can be used for the quick-look analysis of data at the telescope as well as for pipeline reduction of large data sets. COSMOS is based on a precise optical model of the spectrographs, which allows (after alignment and calibration) an accurate prediction of the location of spectra features. This eliminates the line search procedure which is fundamental to many spectral reduction programs, and allows a robust data pipeline to be run in an almost fully automatic mode, allowing large amounts of data to be reduced with minimal intervention.

  6. The Carnegie Commission and Council on Higher Education: A Retrospective. Research and Occasional Paper Series: CSHE.14.05

    ERIC Educational Resources Information Center

    Douglass, John Aubrey

    2005-01-01

    It has been nearly forty years since Clark Kerr was asked to create and lead the Carnegie Commission on Higher Education under the auspices of the Carnegie Corporation. The Commission was to be a national effort, unprecedented both in scope and in the freedom of its director, Kerr, to guide its research and productivity. Carnegie President Alan…

  7. The Carnegie Commission and Council on Higher Education: A Retrospective. Research & Occasional Paper Series. CSHE.14.05

    ERIC Educational Resources Information Center

    Douglass, John Aubrey

    2005-01-01

    It has been nearly forty years since Clark Kerr was asked to create and lead the Carnegie Commission on Higher Education under the auspices of the Carnegie Corporation. The Commission was to be a national effort, unprecedented both in scope and in the freedom of its director, Kerr, to guide its research and productivity. Carnegie President Alan…

  8. Public Speaking on the Streets and in the Ivory Tower: A Comparison of the Dale Carnegie Course and the Academic Course.

    ERIC Educational Resources Information Center

    Miller, Christine M.

    Many speech communication educators and researchers look upon Dale Carnegie's public speaking course with derision for its methods as well as its motives. A comparison of Carnegie's course with university courses in speech communication reveals a number of differences between the two, which in part explains this attitude. Carnegie began his course…

  9. What Young Adolescents Want and Need from Out-of-School Programs: A Focus Group Report.

    ERIC Educational Resources Information Center

    Morris (S. W.) & Company, Inc., Bethesda, MD.

    The Carnegie Council on Adolescent Development undertook a 2-year project to assess non-school programs offered by various community-based youth organizations. This project included focus group interviews with youth about their current activities and preferences for after-school activities. Sixteen focus groups were conducted in the metropolitan…

  10. Balancing Interests: Rethinking U.S. Selection of Skilled Immigrants. International Migration Policy Program 4.

    ERIC Educational Resources Information Center

    Papademetriou, Demetrios G.; Yale-Loehr, Stephen

    The Carnegie Endowment's International Migration Policy Program convened a study group to review and develop alternative approaches to the way foreign workers gain access to the United States through the employment-based immigration stream. This study, a product of that effort, focuses on the selection of people admitted under work-related…

  11. Community College Pathways' Program Success: Assessing the First Two Years' Effectiveness of Statway®

    ERIC Educational Resources Information Center

    Yamada, Hiroyuki

    2014-01-01

    Statway® is one of the Community College Pathways initiatives developed by the Carnegie Foundation for the Advancement of Teaching to promote students' progress beginning in developmental math to and through college math credit. Early descriptive results suggested that the Statway program has tripled the success rate for students in half the time…

  12. Learning to Walk the Talk: Designing a Teacher Leadership EdD Program as a Laboratory of Practice

    ERIC Educational Resources Information Center

    Sawyer, Richard D.

    2013-01-01

    This article tries to "put a face" on the complex and abstract process of program change in relation to key principles from the Carnegie Project on the Education Doctorate (CPED). We examine the principles of the "scholarship of practice," "laboratory of practice," and "signature pedagogy" within a…

  13. 78 FR 48703 - Proposed Flood Hazard Determinations

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-08-09

    ..., Bridgeville, PA 15017. Borough of Carnegie Borough Building, 1 Veterans Way, Carnegie, PA 15106. Borough of.... Township of Scott Scott Township Office, 301 Lindsay Road, Carnegie, PA 15106. Township of Shaler Shaler...

  14. Composing Interfering Abstract Protocols

    DTIC Science & Technology

    2016-04-01

    Tecnologia , Universidade Nova de Lisboa, Caparica, Portugal. This document is a companion technical report of the paper, “Composing Interfering Abstract...a Ciência e Tecnologia (Portuguese Foundation for Science and Technology) through the Carnegie Mellon Portugal Program under grant SFRH / BD / 33765

  15. 48 CFR 235.017-1 - Sponsoring agreements.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ..., DEPARTMENT OF DEFENSE SPECIAL CATEGORIES OF CONTRACTING RESEARCH AND DEVELOPMENT CONTRACTING 235.017-1... Institute of Technology, and Software Engineering Institute operated by Carnegie Mellon) may respond to solicitations and announcements for programs which promote research, development, demonstration, or transfer of...

  16. 48 CFR 235.017-1 - Sponsoring agreements.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ..., DEPARTMENT OF DEFENSE SPECIAL CATEGORIES OF CONTRACTING RESEARCH AND DEVELOPMENT CONTRACTING 235.017-1... Institute of Technology, and Software Engineering Institute operated by Carnegie Mellon) may respond to solicitations and announcements for programs which promote research, development, demonstration, or transfer of...

  17. Low Cost Technical Solutions to Jump Start an Insider Threat Program

    DTIC Science & Technology

    2016-05-11

    Low Cost Technical Solutions to Jump Start an Insider Threat Program George J. Silowash Derrick L. Spooner Daniel L. Costa Michael J...Albrethsen May 2016 TECHNICAL NOTE CMU/SEI-2016-TN-004 CERT Division http://www.sei.cmu.edu Copyright 2016 Carnegie Mellon University This... technical note will explore tools that may be suitable for satisfying the basic technical needs of an insider threat program, giving organizations a

  18. VizieR Online Data Catalog: The Carnegie-Chicago Hubble Program. II. IC 1613 (Hatt+, 2017)

    NASA Astrophysics Data System (ADS)

    Hatt, D.; Beaton, R. L.; Freedman, W. L.; Madore, B. F.; Jang, I.-S.; Hoyt, T. J.; Lee, M. G.; Monson, A. J.; Rich, J. A.; Scowcroft, V.; Seibert, M.

    2018-04-01

    Observations of IC 1613 were obtained on 2015 June 12 using the Inamori-Magellan Areal Camera and Spectrograph (IMACS) on the 6.5m Magellan-Baade telescope at Las Campanas Observatory. We obtain a 15.46'x15.46' field of view with resolution of 0.2"/pixel and observed in the BVI filters. See section 2.1.1. We have made use of archival imaging of IC 1613 taken from the Local Cosmology from Isolated Dwarfs program (PID:GO10505, PI: Gallart; Gallart 2005, LCID). A single field was imaged over 24 orbits between 2006 August 28 and 30 approximately 5' west of the center of IC 1613 using the HST ACS/WFC instrument, which provides a 202"x202" field of view with 0.05"/pixel resolution. Each orbit was divided between two ~1200s exposures in the F475W and F814W passbands, resulting in 48 epochs per filter. See section 2.1.2. We obtained near-infrared imaging over 24 orbits between 2014 December 17 and 18 using the HST WFC3/IR instrument (PID:GO13691, PI: Freedman; Freedman W. 2014 HST Proposal). The orbits were divided between two overlapping 136"x123" WFC3/IR pointings with a native resolution of 0.135"/pixel. See section 2.1.3. In parallel with the observations described in the previous section were 24 orbits with the HST ACS/WFC instrument (PID:GO13691, PI: Freedman; Freedman 2014 W. HST Proposal). Each exposure in F606W and F814W spanned ~500s. See section 2.1.4. (2 data files).

  19. Adolescent Literacy Programs: Costs of Implementation. Final Report from Carnegie Corporation of New York's Council on Advancing Adolescent Literacy

    ERIC Educational Resources Information Center

    Levin, Henry M.; Catlin, Doran; Elson, Alex

    2010-01-01

    Many educators and researchers have proposed reforms for dealing with the ongoing adolescent literacy crisis. Progress in strengthening young people's literacy now depends on schools a) choosing appropriate programs and b) implementing them consistently and effectively. Yet the history of school reform is littered with reforms that were adopted…

  20. Research in Information Processing and Computer Science. Final Technical Report.

    ERIC Educational Resources Information Center

    Carnegie-Mellon Univ., Pittsburgh, PA. Social Studies Curriculum Center.

    This is the final scientific research report for the research in programing at Carnegie-Mellon University during 1968-1970. Three team programing efforts during the past two years have been the development of (1) BLISS--a system building language on the PDP-10 computer, (2) LC2--a conversational system on the IBM/360, and L*--a system building…

  1. A Measurement & Analysis Training Solution Supporting CMMI & Six Sigma Transition

    DTIC Science & Technology

    2004-10-01

    product” • Designing an integrated training solution • Illustration(s) © 2004 by Carnegie Mellon University Version 1.0 page 5 Carnegie Mellon S...12207 Score- card EIA 632 ISO 9000 ITIL COBIT PSM GQIM © 2004 by Carnegie Mellon University Version 1.0 page 7 Carnegie Mellon S oftware Engineer ing...several Capability Maturity Models, reflects Crosby’s 5 maturity levels • Focuses on infrastructure and process maturity • Intended for software and

  2. NASA Astrophysics E/PO: The Impact of the Space Telescope Science Institute Office of Public Outreach

    NASA Astrophysics Data System (ADS)

    Smith, Denise A.; Jirdeh, Hussein; Eisenhamer, Bonnie; Villard, Ray

    2015-01-01

    As the science operations center for Hubble and Webb, the Space Telescope Science Institute (STScI) is uniquely positioned to captivate the imagination and inspire learners of all ages in humanity's quest to understand fundamental questions about our universe and our place in it. With the 25th anniversary of Hubble's launch and deployment approaching in April 2015, this presentation will provide an overview of the impact of the STScI's Office of Public Outreach's programs to engage students, educators, and the public in exploring the universe through audience-based news, education, and outreach programs. At the heart of our programs lies a tight coupling of scientific, education, and communications expertise. By partnering scientists and educators, we assure current, accurate science content and education products and programs that are classroom-ready and held to the highest pedagogical standards. Likewise, news and outreach programs accurately convey cutting-edge science and technology in a way that is attuned to audience needs. The combination of Hubble's scientific capabilities and majestic imagery, together with a deep commitment to creating effective programs to share Hubble science with the education community and the public, has enabled the STScI Office of Public Outreach programs to engage 6 million students and ½ million educators per year, and 24 million online viewers per year. Hubble press releases generate approximately 5,000 online news articles per year with an average circulation of 125 million potential readers per press release news story. We will also share how best practices and lessons learned from this long-lived program are already being applied to engage a new generation of explorers in the science and technology of the James Webb Space Telescope.

  3. National Study of Excellence and Innovation in Physical Therapist Education: Part 1-Design, Method, and Results.

    PubMed

    Jensen, Gail M; Nordstrom, Terrence; Mostrom, Elizabeth; Hack, Laurita M; Gwyer, Janet

    2017-09-01

    The Carnegie Foundation for the Advancement of Teaching commissioned the Preparation for the Professions Program, a qualitative study of professional education in 5 professions: medicine, nursing, law, engineering, and clergy. These studies identified curricular structures, instructional practices, assessment approaches, and environmental characteristics that support the preparation of professionals and led to educational reforms. The physical therapy profession has not had any in-depth, national investigation of physical therapist education since the Catherine Worthingham studies conducted more than 50 years ago. This research was a Carnegie-type study, investigating elements of excellence and innovation in academic and clinical physical therapist education in the United States. Five physical therapist education researchers from across the United States used a qualitative multiple-case study design. Six academic and 5 clinical programs were selected for the study. The academic institutions and clinical agencies studied were diverse in size, institutional setting, geography, and role in residency education. Qualitative case studies were generated from review of artifacts, field observations, and interviews (individual and focus group), and they provided the data for the study. A conceptual framework grounded in 3 major dimensions was generated, with 8 supporting elements: (1) culture of excellence (shared beliefs and values, leadership and vision, drive for excellence, and partnerships), (2) praxis of learning (signature pedagogy, practice-based learning, creating adaptive learners, and professional formation), and (3) organizational structures and resources. Building on the work of the Carnegie Foundation's Preparation for the Professions Program, a conceptual model was developed, representing the dimensions and elements of excellence in physical therapist education that is centered on the foundational importance of a nexus of linked and highly valued aims of being learner centered and patient centered in all learning environments, both academic and clinical. © 2017 American Physical Therapy Association

  4. The Carnegie Mellon/Sirsi Corporation Alliance.

    ERIC Educational Resources Information Center

    Troll, Denise A.; Depellegrin, Tracey A.; Myers, Melanie D.

    1999-01-01

    Describes the relationship between Carnegie Mellon University libraries and Sirsi Corporation, their integrated library-management system vendor. Topics include Carnegie Mellon's expertise in library automation research and development; and three primary elements of the alliance: research, including user protocols, surveys, and focus groups;…

  5. 76 FR 51982 - Agency Forms Undergoing Paperwork Reduction Act Review

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-08-19

    ... Dynamic Decision Making Laboratory at Carnegie Mellon University will investigate several independent... Carnegie Mellon University and the University of Pittsburgh between January 2010 and December 2010. Participants were recruited through an online research participant pool from Carnegie Mellon University and the...

  6. DMPL: Programming and Verifying Distributed Mixed Synchrony and Mixed Critical Software

    DTIC Science & Technology

    2016-06-16

    ference on Intelligent Robots and Systems, pages 1495–1502, Chicago, IL, September 2014. IEEE Computer Society. [21] MADARA website . http://sourceforge.net...4.6 DMPL program for 5- robot reconnaissance example 19 Figure 5.1 Generated C++ code for example DMPL program. In practice, local vari- ables (lines...examples of collision avoidance in multi- robot systems. CMU/SEI-2016-TR-005 | SOFTWARE ENGINEERING INSTITUTE | Carnegie Mellon University vii

  7. Report from the First CERT-RMM Users Group Workshop Series

    DTIC Science & Technology

    2012-04-01

    deploy processes to support our programs – Benchmark our programs to determine current gaps – Complements current work in CMMI® and ISO 27001 19...benchmarking program performance through process analytics and Lean/Six Sigma activities to ensure Performance Excellence. • Provides ISO Standards...Office www.cmu.edu/ iso 29 Carnegie Mellon University • Est 1967 in Pittsburgh, PA • Global, private research university • Ranked 22nd • 15,000

  8. How Community Colleges Understand the Scholarship of Teaching and Learning.

    ERIC Educational Resources Information Center

    Sperling, Charmian B.

    2003-01-01

    Describes the involvement of Middlesex Community College, Massachusetts, in the Carnegie Teaching Academy program. Faculty and staff at the college broadened their understanding of instructional pedagogy through greater appreciation of relevant connections between learning theory and classroom practice. Argues that faculty scholarship ultimately…

  9. Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program

    NASA Astrophysics Data System (ADS)

    Simon, Amy

    2017-08-01

    Long time base observations of the outer planets are critical in understanding the atmospheric dynamics and evolution of the gas giants. We propose yearly monitoring of each giant planet for the remainder of Hubble's lifetime to provide a lasting legacy of increasingly valuable data for time-domain studies. The Hubble Space Telescope is a unique asset to planetary science, allowing high spatial resolution data with absolute photometric knowledge. For the outer planets, gas/ice giant planets Jupiter, Saturn, Uranus and Neptune, many phenomena happen on timescales of years to decades, and the data we propose are beyond the scope of a typical GO program. Hubble is the only platform that can provide high spatial resolution global studies of cloud coloration, activity, and motion on a consistent time basis to help constrain the underlying mechanics.

  10. "PROPAGANDISTS FOR THE BEHAVIORAL SCIENCES": THE OVERLOOKED PARTNERSHIP BETWEEN THE CARNEGIE CORPORATION AND SSRC IN THE MID-TWENTIETH CENTURY.

    PubMed

    Hauptmann, Emily

    2016-01-01

    The Carnegie Corporation's role as a patron of the behavioral sciences has been overlooked; its support for the behavioral sciences not only began earlier than the Ford Foundation's but was also at least equally important to their success. I show how the close postwar collaboration between the Carnegie Corporation and the Social Science Research Council (SSRC) to promote the behavioral sciences emerged after a struggle between Carnegie and the Rockefeller Foundation over the direction and leadership of the SSRC. I then focus on three postwar projects Carnegie helped conceive and fund that were publicized as the work of the SSRC: Chase's The Proper Study of Mankind (1948), Stouffer et al.'s The American Soldier (), and the Michigan's Survey Research Center 1952 election study. In each of these projects, Carnegie deliberately muted its own role and promoted the remade SSRC as a major advocate for the behavioral sciences. © 2016 Wiley Periodicals, Inc.

  11. The Role of Sports in Youth Development. Report of a meeting convened by Carnegie Corporation of New York (March 18, 1996).

    ERIC Educational Resources Information Center

    Poinsett, Alex

    This document summarizes a conference on the potential impact of sports on at-risk youngsters. More than 40 scholars and practitioners met to explore the role that sports programs play in promoting academic success, health and fitness, responsible social behaviors, and self-confidence, and ways that such programs could be expanded to reach those…

  12. Anomaly Detection and Modeling of Trajectories

    DTIC Science & Technology

    2012-08-01

    policies, either expressed or implied, of the Gates Millennium Scholars Program , or the Office of Naval Research. Report Documentation Page Form... PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT NUMBER 5e. TASK NUMBER 5f. WORK UNIT NUMBER 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) Carnegie...thesis proposes several methods using statistics and machine learning (ML) that provide a deep understanding of trajectory datasets. In particular

  13. 76 FR 21906 - Proposed Data Collections Submitted for Public Comment and Recommendations

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-04-19

    ... at Carnegie Mellon University will investigate several independent variables relevant to Instance... Laboratory conducted this research with a total of 28 students from Carnegie Mellon University and the... online research participant pool from Carnegie Mellon University and the University of Pittsburgh to...

  14. Calibration of the Hubble Space Telescope polarimetric modes

    NASA Technical Reports Server (NTRS)

    Lupie, O. L.; Stockman, H. S.

    1988-01-01

    Stellar and galactic polarimetry from space is an unexplored observational regime and one which holds exciting promise for answering many fundamental astrophysical questions. The Hubble Space Telescope will be the first space observatory to provide a variety of polarimetric modes to astronomers including spectral, imaging, and single-aperture UV polarimetry. As part of the calibration program for these modes, the Space Telescope Science Institute has initiated a ground-based program to define faint standard fields and solicited community support to establish a temporal baseline for these potential standard targets. In this paper, the polarimetric capabilities of the Hubble Space Telescope, the philosophy and complications of in-flight calibration, and the status and direction of the standard targets program are discussed.

  15. Reflections on Doctoral Education in Chemistry. Carnegie Essays on the Doctorate: Chemistry.

    ERIC Educational Resources Information Center

    Kwiram, Alvin L.

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  16. The Ph.D. in Education. Carnegie Essays on the Doctorate: Education.

    ERIC Educational Resources Information Center

    Richardson, Virginia

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  17. The Doctorate in Chemistry. Carnegie Essays on the Doctorate: Chemistry.

    ERIC Educational Resources Information Center

    Breslow, Ronald

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  18. Carnegie Cuts a Crater

    NASA Image and Video Library

    2015-04-10

    Carnegie Rupes makes a dramatic sight in this large image mosaic. The giant lobate scarp cuts through Duccio crater. If you were to approach the scarp from the southwest, you would find yourself facing a wall nearly 2 km high! Be sure to zoom in for a closer look! Carnegie Rupes was named after a research vessel launched in 1909. The ship was built almost entirely from wood and other non-magnetic materials to allow sensitive magnetic measurements to be taken for the Carnegie Institution's Department of Terrestrial Magnetism. http://photojournal.jpl.nasa.gov/catalog/PIA19279

  19. Causality-Preserving Timestamps in Distributed Programs

    DTIC Science & Technology

    1993-06-01

    monitoring,deh!bigging. tac-hvon,catisaIi tvý Abstract A tachyon is an improperly ordered event in a distributed program. Tachvonis are most often...that tachyons do in fact. occur commonly in distributed pro- grams on our Ethernet at Carnegie Mellon University. and we disc’ss some ways of...before it is sent) is called a tach yon. (’learly it is very disconcerting to try to debug a parallel program that contains tachyons . Of course, in "real

  20. FRONTIER FIELDS: HIGH-REDSHIFT PREDICTIONS AND EARLY RESULTS

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Coe, Dan; Bradley, Larry; Zitrin, Adi, E-mail: DCoe@STScI.edu

    2015-02-20

    The Frontier Fields program is obtaining deep Hubble and Spitzer Space Telescope images of new ''blank'' fields and nearby fields gravitationally lensed by massive galaxy clusters. The Hubble images of the lensed fields are revealing nJy sources (AB mag > 31), the faintest galaxies yet observed. The full program will transform our understanding of galaxy evolution in the first 600 million years (z > 9). Previous programs have yielded a dozen or so z > 9 candidates, including perhaps fewer than expected in the Ultra Deep Field and more than expected in shallower Hubble images. In this paper, we present high-redshift (z >more » 6) number count predictions for the Frontier Fields and candidates in three of the first Hubble images. We show the full Frontier Fields program may yield up to ∼70 z > 9 candidates (∼6 per field). We base this estimate on an extrapolation of luminosity functions observed between 4 < z < 8 and gravitational lensing models submitted by the community. However, in the first two deep infrared Hubble images obtained to date, we find z ∼ 8 candidates but no strong candidates at z > 9. We defer quantitative analysis of the z > 9 deficit (including detection completeness estimates) to future work including additional data. At these redshifts, cosmic variance (field-to-field variation) is expected to be significant (greater than ±50%) and include clustering of early galaxies formed in overdensities. The full Frontier Fields program will significantly mitigate this uncertainty by observing six independent sightlines each with a lensing cluster and nearby blank field.« less

  1. A Long Shadow: Frederick P. Keppel, the Carnegie Corporation and the Dominions and Colonies Fund Area Experts 1923-1943

    ERIC Educational Resources Information Center

    Glotzer, Richard

    2009-01-01

    The Carnegie Corporation found its first great manager in Frederick Paul Keppel (1875-1943). Keppel's career is important to historians of education because interwar Carnegie initiatives, articulated through the Corporation's Dominions and Colonies Fund and Teachers College, Columbia University, internationalised American educational theories and…

  2. Case Study IV: Carnegie Foundation for the Advancement of Teaching's Networked Improvement Communities (NICs)

    ERIC Educational Resources Information Center

    Coburn, Cynthia E.; Penuel, William R.; Geil, Kimberly E.

    2015-01-01

    The Carnegie Foundation for the Advancement of Teaching is a nonprofit, operating foundation with a long tradition of developing and studying ways to improve teaching practice. For the past three years, the Carnegie Foundation has initiated three different Networked Improvement Communities (NICs). The first, Quantway, is addressing the high…

  3. The Carnegie Unit: A Century-Old Standard in a Changing Education Landscape

    ERIC Educational Resources Information Center

    Silva, Elena; White, Taylor; Toch, Thomas

    2015-01-01

    Early in the twentieth century, the industrialist Andrew Carnegie established the Carnegie Foundation for the Advancement of Teaching to create a pension system for the nation's college professors. The introduction of this pension system proved an ingenious educational reform. At the time, American higher education was a largely ill-defined…

  4. Integrating Interview Methodology to Analyze Inter-Institutional Comparisons of Service-Learning within the Carnegie Community Engagement Classification Framework

    ERIC Educational Resources Information Center

    Plante, Jarrad D.; Cox, Thomas D.

    2016-01-01

    Service-learning has a longstanding history in higher education in and includes three main tenets: academic learning, meaningful community service, and civic learning. The Carnegie Foundation for the Advancement of Teaching created an elective classification system called the Carnegie Community Engagement Classification for higher education…

  5. Engaged with Carnegie: Effects of Carnegie Classification Recognition on CUMU Universities

    ERIC Educational Resources Information Center

    Arfken, Deborah Elwell; Ritz, Susan

    2013-01-01

    This paper provides the results of a survey sent to all thirty-two CUMU institutions that have received the Carnegie recognition and specifically examines a) reasons for applying for the elective classification; b) level of pride instilled in campuses; and c) level of impact on institutional identity and culture, institutional commitment,…

  6. Imagine There's No Carnegie Unit

    ERIC Educational Resources Information Center

    Klevgaard, Janine

    2013-01-01

    This article describes how the Alberta Education High School Flexibility Enhancement Pilot Project allowed 16 high schools in Alberta, Canada, to remove the restrictions of the Carnegie unit, the seat time per credit requirement that has been widely used since 1906. The two purposes of the project were to determine whether the Carnegie unit should…

  7. Educational Reforms and Ethical Use of Research to Inform Readers

    ERIC Educational Resources Information Center

    Turgut, Guliz

    2013-01-01

    This article critique reflects on "Standards for a New Century: Educating U.S. Students to Compete in the Global Economy," which was published in 2009 in the "Carnegie Reporter", a publication of The Carnegie Corporation of New York. The article, written by Carnegie staff writer Karen Theroux, explained the need for Common Core…

  8. The Mathematics Doctorate: A Time for Change? Carnegie Essays on the Doctorate: Mathematics.

    ERIC Educational Resources Information Center

    Chan, Tony F.

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  9. Words and Responsibilities: Graduate Education and the Humanities. Carnegie Essays on the Doctorate: Humanities.

    ERIC Educational Resources Information Center

    Stimpson, Catharine R.

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  10. The Ph.D. in English: Towards a New Consensus. Carnegie Essays on the Doctorate: English.

    ERIC Educational Resources Information Center

    Graff, Gerald

    The Carnegie Foundation commissioned a collection of essays as part of the Carnegie Initiative on the Doctorate (CID). Essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. Intended to engender conversation about the conceptual foundation of doctoral…

  11. Frederick P. Keppel and the Carnegie Corporation's Interwar Area Experts: An Overview

    ERIC Educational Resources Information Center

    Glotzer, Richard

    2006-01-01

    Under the leadership of Frederick Paul Keppel (1875-1943) Carnegie Corporation's Dominions and Colonies Fund supported a vast array of philanthropic projects in the dominions and colonies of the Britain's interwar empire. The career of F. P. Keppel is important to historians of education because many of the interwar Carnegie initiatives…

  12. The ALICE System: A Workbench for Learning and Using Language.

    ERIC Educational Resources Information Center

    Levin, Lori; And Others

    1991-01-01

    ALICE, a multimedia framework for intelligent computer-assisted language instruction (ICALI) at Carnegie Mellon University (PA), consists of a set of tools for building a number of different types of ICALI programs in any language. Its Natural Language Processing tools for syntactic error detection, morphological analysis, and generation of…

  13. Undergraduate Education in Science: A Rationale for Program Structure.

    ERIC Educational Resources Information Center

    National Science Foundation, Washington, DC.

    This publication encompasses the central core of the National Science Foundation's (NSF) explicit science education activities at the undergraduate level of the Nation's education enterprise. It is an outline of the character of the Foundation's educational constituency. A table is presented showing the Carnegie Commission's Classification Scheme…

  14. The Dissertation in Practice: A Student's Perspective

    ERIC Educational Resources Information Center

    Stacy, Jaime C.

    2013-01-01

    This article describes the impact that coursework related to Virginia Commonwealth University's inaugural EdD program had on a public school administrator; particularly how the Carnegie Project for the Educational Doctorate's (CPED) working principles continue to play a role in solving "Problems of Practice" in an at-risk school long…

  15. NSF Says It Will Support Supercomputer Centers in California and Illinois.

    ERIC Educational Resources Information Center

    Strosnider, Kim; Young, Jeffrey R.

    1997-01-01

    The National Science Foundation will increase support for supercomputer centers at the University of California, San Diego and the University of Illinois, Urbana-Champaign, while leaving unclear the status of the program at Cornell University (New York) and a cooperative Carnegie-Mellon University (Pennsylvania) and University of Pittsburgh…

  16. Making the Most of Libraries in the Search for Academic Excellence.

    ERIC Educational Resources Information Center

    Breivik, Patricia Senn

    1987-01-01

    The role of libraries in the search for quality education was addressed in the Carnegie Foundation's report, "College," and at the first higher education conference on academic libraries. Information literacy and policy, campus organizational issues, and programs in economic development support, active learning, and faculty development…

  17. The Hubble Space Telescope at 25: Lessons Learned for Future Missions

    NASA Astrophysics Data System (ADS)

    Wiseman, Jennifer

    2015-08-01

    This year we celebrate the 25th anniversary of the Hubble Space Telescope mission. Astronomy worldwide has been transformed by the discoveries made with Hubble. At this momentous milestone it is important to reflect on the unique successes of Hubble, and the components of that success, as the astronomical community develops facilities and a vision for future major international efforts in scientific space exploration. First, Hubble was envisioned by pioneering astronomers long before its launch, galvanizing support from astronomers, NASA, and governmental leaders for such an innovative and risky endeavor. Second, the interplay of the astronaut program with scientific exploration was paramount to the success of Hubble, not only with the initial dramatic repair mission, but also for the subsequent five servicing missions that kept the observatory perpetually refreshed. Cooperative missions involving astronauts, engineers, and scientists may be critical for constructing and operating large facilities in space in the future. Third, the scientific discoveries of Hubble involve both incredible successes that were planned from the outset as well as new discoveries and innovative uses of the observatory that could not have been planned in advance. Hubble has been used not only to gauge the expansion rate and age of the universe, but has also been a major player in the recent surprise detection of acceleration in that expansion. Hubble has also been key for studying star formation and now the atmospheres of exoplanets; even water has been detected in exoplanetary systems, something never envisioned for Hubble originally. And the incredible evolutionary picture of galaxies has been unveiled through Hubble observations, now enhanced by the revolutionary uses of gravitational lensing to study both dark matter in the lensing clusters, and extremely distant magnified galaxies. Finally, Hubble’s great success in public outreach has made the discoveries of astronomy easily accessible and treasured by people around the world. This talk will outline how these successes of the Hubble Space Telescope program can inform and prepare us for future large scale astronomical facilities and exploration endeavors.

  18. The Online Credit Hour: A Brief History and Guide to Regional Accreditation Similarities, Differences, and How They Can Affect Your Programs

    ERIC Educational Resources Information Center

    Schulte, Marthann

    2016-01-01

    In this article, the author first traces the history of what is today known as the "Carnegie Unit" or course credit and discusses how it has become improperly equated with learning and abused in online and for-profit programs. The second half of the article provides statements concerning online credit hours from the following regional…

  19. Quantifying the Hurricane Risk to Offshore Wind Power (Invited)

    NASA Astrophysics Data System (ADS)

    Apt, J.; Rose, S.; Jaramillo, P.; Small, M.

    2013-12-01

    The U.S. Department of Energy has estimated that over 50 GW of offshore wind power will be required for the United States to generate 20% of its electricity from wind. Developers are actively planning offshore wind farms along the U.S. Atlantic and Gulf coasts and several leases have been signed for offshore sites. These planned projects are in areas that are sometimes struck by hurricanes. Whether that risk will grow as a result of climate change is uncertain. Recent years have seen an increase in hurricane activity in the Atlantic basin (1) and, all else being equal, warmer sea surface temperatures can be expected to lead to increased storm intensity. We have developed a method to estimate the catastrophe risk to offshore wind power using simulated hurricanes (2). In Texas, the most vulnerable region we studied, 10% of offshore wind power could be offline simultaneously due to hurricane damage with a 100-year return period and 6% could be destroyed in any 10-year period. Much of the hurricane risk to offshore wind turbines can be mitigated by designing turbines for higher maximum wind speeds, ensuring that turbine nacelles can turn quickly to track the wind direction even when grid power is lost, and building in areas with lower risk. 1. Iris Grossmann and M. Granger Morgan, "Tropical Cyclones, Climate Change, and Scientific Uncertainty: What do we know, what does it mean, and what should be done?," Climatic Change, 108, pp 543-579, 2011. 2. Carnegie Mellon Electricity Industry Center Working Paper CEIC-13-07, http://wpweb2.tepper.cmu.edu/electricity/papers/ceic-13-07.asp This work was supported in part by the EPA STAR fellowship program, a grant from the Alfred P. Sloan Foundation and EPRI to the Carnegie Mellon Electricity Industry Center, and by the Doris Duke Charitable Foundation, the R.K. Mellon Foundation and the Heinz Endowments for support of the RenewElec program at Carnegie Mellon University. This research was also supported in part by the Climate and Energy Decision Making (CEDM) center created through a cooperative agreement between the National Science Foundation (SES-0949710) and Carnegie Mellon University.

  20. Carnegie Math Pathways 2015-2016 Impact Report: A Five-Year Review. Carnegie Math Pathways Technical Report

    ERIC Educational Resources Information Center

    Hoang, Hai; Huang, Melrose; Sulcer, Brian; Yesilyurt, Suleyman

    2017-01-01

    College math is a gateway course that has become a constraining gatekeeper for tens of thousands of students annually. Every year, over 500,000 students fail developmental mathematics, preventing them from achieving their college and career goals. The Carnegie Math Pathways initiative offers students an alternative. It comprises two Pathways…

  1. The Carnegie Council on Policy Studies in Higher Education: A Summary of Reports and Recommendations.

    ERIC Educational Resources Information Center

    Carnegie Council on Policy Studies in Higher Education, Berkeley, CA.

    Work of the Carnegie Council on Policy Studies in Higher Education, which began in 1974 and concluded its work in January 1980, is reported. The Council's 15 policy reports and 38 sponsored research and technical reports are summarized. A paper entitled "The Carnegie Policy Series, 1967-1979: Concerns, Approaches, Reconsiderations,…

  2. Libraries and Andrew Carnegie's Challenge.

    ERIC Educational Resources Information Center

    Gregorian, Vartan

    This essay by the president of the Carnegie Corporation of New York (reprinted from the 1998 annual report) opens by noting that the year 1999 marks the 100th anniversary of Andrew Carnegie's support for the planning and development of 65 branch libraries of the New York Public Library System, a gift that came to more than $5.2 million. Discussion…

  3. Comparing the Utility of the 2000 and 2005 Carnegie Classification Systems in Research on Students' College Experiences and Outcomes

    ERIC Educational Resources Information Center

    McCormick, Alexander C.; Pike, Gary R.; Kuh, George D.; Chen, Pu-Shih Daniel

    2009-01-01

    This study compares the explanatory power of the 2000 edition of Carnegie Classification, the 2005 revision of the classification, and selected variables underlying Carnegie's expanded 2005 classification system using data from the National Survey of Student Engagement's spring 2004 administration. Results indicate that the 2000 and 2005…

  4. Rethinking the Ph.D. in English. Carnegie Essays on the Doctorate: English.

    ERIC Educational Resources Information Center

    Lunsford, Andrea Abernethy

    The Carnegie Foundation commissioned a series of essays as part of the Carnegie Initiative on the Doctorate (CID). The essays and essayists represent six disciplines that are part of the CID: chemistry, education, English, history, mathematics, and neuroscience. The essay explores the Ph.D. in English and suggests changes the author would make in…

  5. Lessons Learned from the Hubble Space Telescope (HST) Contamination Control Program

    NASA Technical Reports Server (NTRS)

    Hansen, Patricia A.; Townsend, Jacqueline A.; Hedgeland, Randy J.

    2004-01-01

    Over the past two decades, the Hubble Space Telescope (HST) Contamination Control Program has evolved from a ground-based integration program to a space-based science-sustaining program. The contamination controls from the new-generation Scientific Instruments and Orbital Replacement Units were incorporated into the HST Contamination Control Program to maintain scientific capability over the life of the telescope. Long-term on-orbit scientific data has shown that these contamination controls implemented for the instruments, Servicing Mission activities (Orbiter, Astronauts, and mission), and on-orbit operations successfully protected the HST &om contamination and the instruments from self-contamination.

  6. Lessons Learned from the Hubble Space Telescope (HST) Contamination Control Program

    NASA Technical Reports Server (NTRS)

    Hansen, Patricia A.; Townsend, Jacqueline A.; Hedgeland, Randy J.

    2004-01-01

    Over the past two decades, the Hubble Space Telescope (HST) Contamination Control Program has evolved from a ground-based integration program to a space-based science-sustaining program. The contamination controls from the new-generation Scientific Instruments and Orbital Replacement Units were incorporated into the HST Contamination Control Program to maintain scientific capability over the life of the telescope. Long-term on-orbit scientific data has shown that these contamination controls implemented for the instruments, Servicing Mission activities (Orbiter, Astronauts, and mission), and on-orbit operations successfully protected the HST from contamination and the instruments from self-contamination.

  7. Enacting the Carnegie Foundation call for reform of medical school and residency.

    PubMed

    O'Brien, Bridget C; Irby, David M

    2013-01-01

    On the 100th anniversary of the Flexner Report, the Carnegie Foundation for the Advancement of Teaching published a new study of medical education. This study, titled Educating Physicians: A Call for Reform of Medical Schools and Residency Programs, contained four primary recommendations intended to stimulate innovation and improvement in medical education. In this article, the authors examined the ways others have applied the four recommendations from Educating Physicians within and beyond medical education. In their review of 246 publications citing the Carnegie work, they found that the recommendation for integration was addressed most frequently, often through descriptions of integration of curricular content in undergraduate medical education. The recommendation to focus on professional identity formation was the second most frequently addressed, followed by standardization and individualization, then inquiry, innovation, and improvement. The publications related to these latter three recommendations tended to be conceptual rather than descriptive or empirical. Publications spanned the continuum of medical education (from medical school to residency to physicians in practice) and even into other fields, but undergraduate medical education received the most attention. The authors discuss common themes among the citing publications and highlight opportunities for further discussion and innovation. Many exciting developments have occurred in medical education and beyond since the publication of Educating Physicians in 2010. Thus far, most of the publications citing the Carnegie recommendations describe incremental changes in medical education, particularly in the area of integration. Some of the conceptual work around these recommendations, coupled with a variety of external factors such as changes in health care and accreditation systems, suggests the potential for changes that are more transformative in nature.

  8. The Archives of the Department of Terrestrial Magnetism: Documenting 100 Years of Carnegie Science

    NASA Astrophysics Data System (ADS)

    Hardy, S. J.

    2005-12-01

    The archives of the Department of Terrestrial Magnetism (DTM) of the Carnegie Institution of Washington document more than a century of geophysical and astronomical investigations. Primary source materials available for historical research include field and laboratory notebooks, equipment designs, plans for observatories and research vessels, scientists' correspondence, and thousands of expedition and instrument photographs. Yet despite its history, DTM long lacked a systematic approach to managing its documentary heritage. A preliminary records survey conducted in 2001 identified more than 1,000 linear feet of historically-valuable records languishing in dusty, poorly-accessible storerooms. Intellectual control at that time was minimal. With support from the National Historical Publications and Records Commission, the "Carnegie Legacy Project" was initiated in 2003 to preserve, organize, and facilitate access to DTM's archival records, as well as those of the Carnegie Institution's administrative headquarters and Geophysical Laboratory. Professional archivists were hired to process the 100-year backlog of records. Policies and procedures were established to ensure that all work conformed to national archival standards. Records were appraised, organized, and rehoused in acid-free containers, and finding aids were created for the project web site. Standardized descriptions of each collection were contributed to the WorldCat bibliographic database and the AIP International Catalog of Sources for History of Physics. Historic photographs and documents were digitized for online exhibitions to raise awareness of the archives among researchers and the general public. The success of the Legacy Project depended on collaboration between archivists, librarians, historians, data specialists, and scientists. This presentation will discuss key aspects (funding, staffing, preservation, access, outreach) of the Legacy Project and is aimed at personnel in observatories, research institutes, and other organizations interested in establishing their own archival programs.

  9. Digital Encounters: Using Information Technology in an Overseas Branch Campus

    ERIC Educational Resources Information Center

    Reilly, Benjamin

    2008-01-01

    In fall of 2004, Carnegie Mellon University embarked on a bold educational experiment, the establishment of an overseas branch campus at Education City in the Persian Gulf state of Qatar. Carnegie Mellon's decision to open up shop in the Middle East was by no means unique; indeed, Carnegie Mellon is just one of a growing number of institutions to…

  10. A Requirement Specification Language for AADL

    DTIC Science & Technology

    2016-06-01

    008 | SOFTWARE ENGINEERING INSTITUTE | CARNEGIE MELLON UNIVERSITY Distribution Statement A: Approved for Public Release; Distribution is Unlimited...Copyright 2016 Carnegie Mellon University This material is based upon work funded and supported by the Department of Defense under Contract No...FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software Engineer- ing Institute, a federally funded research and development

  11. Integrating Trends in Decision-Making Research

    DTIC Science & Technology

    2016-03-01

    Address correspondence to Cleotilde Gonzalez, Department of Social and Decision Sciences, Dynamic Decision Making Lab, Carnegie Mellon University...Cleotilde Gonzalez, Carnegie Mellon University, and Joachim Meyer, Tel-Aviv University Journal of Cognitive Engineering and Decision Making 201X, Volume XX...Number X, Month 2016, pp. 1 –3 DOI: 10.1177/1555343416655256 Copyright © 2016, Human Factors and Ergonomics Society. at CARNEGIE MELLON UNIV LIBRARY

  12. "Turning Points" Revisited: How Effective Middle-Grades Schools Address Developmental Needs of Young Adolescent Students.

    ERIC Educational Resources Information Center

    Martin, Terry

    1993-01-01

    Reviews the Carnegie Council on Adolescent Development Task Force Report (1989) "Turning Points" and looks at some successful middle school programs. Some issues discussed are diversity; self-deveelopment and self-definition; student participation; school and community; social interaction; school climate; and curriculum and instruction.…

  13. Easing the Transition to Middle Adolescence: Educational Implications

    ERIC Educational Resources Information Center

    Beland, Kathy

    2014-01-01

    Mitigating the perils of transition to early adolescence, while also supporting the promise of this stage of human development, has been a major focus of middle school reform (Carnegie Council on Adolescent Development, 1989; Jackson & Davis, 2000). As a result, there are many classroom-based educational programs that target the social and…

  14. Examining CPED Cohort Dissertations: A Window into the Learning of EdD Students

    ERIC Educational Resources Information Center

    Chan, Elaine; Heaton, Ruth M.; Swidler, Stephen A.; Wunder, Susan

    2013-01-01

    Through analyses of three dissertations completed by graduates of our Carnegie Project for the Education Doctorate-influenced program, this article offers insights into both the doctoral students' inquiries into their problems of practice and their faculty advisors' roles and expectations for them. Studying student dissertations provided the…

  15. Change and Sustain/Ability: A Program Director's Reflections on Institutional Learning

    ERIC Educational Resources Information Center

    Asera, Rose

    2008-01-01

    Strengthening Pre-collegiate Education in Community Colleges (SPECC) was organized by The Carnegie Foundation for the Advancement of Teaching in partnership with The William and Flora Hewlett Foundation to increase student learning in developmental--or basic skills--classes. However, their concern was not just the success of students in classes…

  16. Time on Test, Student Motivation, and Performance on the Collegiate Learning Assessment: Implications for Institutional Accountability

    ERIC Educational Resources Information Center

    Hosch, Braden J.

    2010-01-01

    Using results from the Collegiate Learning Assessment (CLA) administered at Central Connecticut State University, a public Carnegie master's-larger programs university in the Northeast, this study demonstrates time on spent on the test, student motivation, and to a lesser extent the local institutional administration procedures represent…

  17. Area Health Education Centers: The Pioneering Years, 1972-1978.

    ERIC Educational Resources Information Center

    Odegaard, Charles E.

    Federal policies and contracts relating to Area Health Education Centers are examined. The evolution of federal programs in the health field is traced, including a discussion of the Carnegie Commission's special reports, the Comprehensive Health Manpower Training Act of 1971, and subsequent amendments to the Act. A detailed outline of the…

  18. Mentor-Mentee Relationship in an Educational Leadership Doctoral Program at Lynn University

    ERIC Educational Resources Information Center

    Reedy, Katherine; Taylor-Dunlop, Korynne

    2015-01-01

    Lynn University embraces the Carnegie Project on the Education Doctorate (CPED) initiative, signature pedagogies and the development of scholarly practitioners. In response to the evolution of educational leadership, Lynn University values the need for doctoral candidates to understand the group process and to be able to work within a diverse…

  19. Library Signage: Applications for the Apple Macintosh and MacPaint.

    ERIC Educational Resources Information Center

    Diskin, Jill A.; FitzGerald, Patricia

    1984-01-01

    Describes specific applications of the Macintosh computer at Carnegie-Mellon University Libraries, where MacPaint was used as a flexible, easy to use, and powerful tool to produce informational, instructional, and promotional signage. Profiles of system hardware and software, an evaluation of the computer program MacPaint, and MacPaint signage…

  20. Leveraging Cababilities of the National Laboratories and Academia to Understand the Properties of Warm Dense MgSiO3

    NASA Astrophysics Data System (ADS)

    Mattsson, Thomas R.; Townsend, Joshua P.; Shulenburger, Luke; Seagle, Christopher T.; Furnish, Michael D.; Fei, Yingwei

    2017-06-01

    For the past seven years, the Z Fundamental Science program has fostered collaboration between scientists at the national laboratories and academic research groups to utilize the Z-machine to explore properties of matter in extreme conditions. A recent example of this involves a collaboration between the Carnegie institution of Washington and Sandia to determine the properties of warm dense MgSiO3 by performing shock experiments using the Z-machine. To reach the higher densities desired, bridgmanite samples are being fabricated at Carnegie using multi-anvil presses. We will describe the preparations under way for these experiments, including pre-shot ab-initio calculations of the Hugoniot and the deployment of dual-layer flyer plates that allow for the measurement of sound velocities along the Hugoniot. Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.

  1. Creation of the Hubble Space Telescope

    NASA Astrophysics Data System (ADS)

    O'Dell, C. R.

    2009-08-01

    The Hubble Space Telescope has been the most successful space astronomy project to date, producing images that put the public in awe and images and spectra that have produced many scientific discoveries. It is the natural culmination of a dream envisioned when rocket flight into space was first projected and a goal set for the US space program soon after NASA was created. The design and construction period lasted almost two decades and its operations have already lasted almost as long. The capabilities of the observatory have evolved and expanded with periodic upgrading of its instrumentation, thus realizing the advantages of its unique design. The success of this long-lived observatory is closely tied to the availability of the Space Shuttle and the end of the Shuttle program means that the end of the Hubble program will follow before long.

  2. RFP Patterns and Techniques for Successful Agile Contracting

    DTIC Science & Technology

    2016-11-01

    2016-SR-025 SOFTWARE ENGINEERING INSTITUTE | CARNEGIE MELLON UNIVERSITY [Distribution Statement A] This material has been approved for public...release and unlimited distribution. Please see Copyright notice for non-U.S. Government use and distribution. Copyright 2016 Carnegie Mellon University...This material is based upon work funded and supported by the Department of Defense under Contract No. FA8721-05-C-0003 with Carnegie Mellon

  3. Energy Harvesting for Soft-Matter Machines and Electronics

    DTIC Science & Technology

    2016-06-09

    AFRL-AFOSR-VA-TR-2016-0353 Energy Harvesting for Soft-Matter Machines and Electronics Carmel Majidi CARNEGIE MELLON UNIVERSITY Final Report 06/09...ES) CARNEGIE MELLON UNIVERSITY 5000 FORBES AVENUE PITTSBURGH, PA 15213-3815 US 8. PERFORMING ORGANIZATION REPORT NUMBER 9. SPONSORING/MONITORING...livelink.ebs.afrl.af.mil/livelink/llisapi.dll DISTRIBUTION A: Distribution approved for public release. Carnegie Mellon University MECHANICAL ENGINEERING FINAL

  4. Using Honeynets and the Diamond Model for ICS Threat Analysis

    DTIC Science & Technology

    2016-05-11

    TR-006 | SOFTWARE ENGINEERING INSTITUTE | CARNEGIE MELLON UNIVERSITY Distribution Statement A: Approved for Public Release; Distribution is...Unlimited Copyright 2016 Carnegie Mellon University This material is based upon work funded and supported by Department of Homeland Security under Contract...No. FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software Engineering Institute, a federally funded research and

  5. Carnegie Corporation's Youth Intergroup Relations Initiative. Report of a Meeting Convened by Carnegie Corporation of New York (New York, NY, October 15-17, 1997).

    ERIC Educational Resources Information Center

    Brawarsky, Sandee

    The Carnegie Corporation's initiative, established in 1996 to create a "new generation of tolerance," included grants to 16 institutions for cutting-edge research in various social science disciplines. Some themes are presented from the second meeting of project leaders for these research efforts. Most of the themes relate to the roles…

  6. The Use of Multilevel Modeling to Estimate Which Measures Are Most Influential in Determining an Institution's Placement in Carnegie's New Doctoral/Research University Classification Schema

    ERIC Educational Resources Information Center

    Micceri, Theodore

    2007-01-01

    This research sought to determine whether any measure(s) used in the Carnegie Foundation's classification of Doctoral/Research Universities contribute to a greater degree than other measures to final rank placement. Multilevel Modeling (MLM) was applied to all eight of the Carnegie Foundation's predictor measures using final rank…

  7. '[T]hen along Comes Mr Carnegie': Carnegie Travel Fellowships and the Professional Development of Kindergarteners in 1930s New Zealand

    ERIC Educational Resources Information Center

    Bethell, Kerry

    2018-01-01

    This article chronicles the experiences of four New Zealand kindergarten teachers who, between 1932 and 1937, were individually awarded Carnegie Corporation of New York Travel Fellowships to undertake an academic year of advanced study at the progressive Teachers College at Columbia University in New York and to visit educational provisions in…

  8. Applying the Goal-Question-Indicator-Metric (GQIM) Method to Perform Military Situational Analysis

    DTIC Science & Technology

    2016-05-11

    www.sei.cmu.edu CMU/SEI-2016-TN-003 | SOFTWARE ENGINEERING INSTITUTE | CARNEGIE MELLON UNIVERSITY Distribution Statement A: Approved for Public Release...Distribution is Unlimited Copyright 2016 Carnegie Mellon University This material is based upon work funded and supported by the Department of...Defense under Contract No. FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software Engineering Institute, a federally

  9. Creating Centralized Reporting for Microsoft Host Protection Technologies:The Enhanced Mitigation Experience Toolkit (EMET)

    DTIC Science & Technology

    2016-08-11

    INSTITUTE | CARNEGIE MELLON UNIVERSITY [Distribution Statement A] This material has been approved for public release and unlimited distribution...Copyright 2016 Carnegie Mellon University This material is based upon work funded and supported by the Department of Defense under Contract No. FA8721...05-C-0003 with Carnegie Mellon University for the operation of the Software Engineer- ing Institute, a federally funded research and development

  10. Evolutionary Systems Design: Recognizing Changes in Security and Survivability Risks

    DTIC Science & Technology

    2006-09-01

    Unlimited distribution subject to the copyright. Technical Note CMU/SEI-2006-TN-027 The Software Engineering Institute is a federally...CARNEGIE MELLON UNIVERSITY AND SOFTWARE ENGINEERING INSTITUTE MATERIAL IS FURNISHED ON AN “AS-IS” BASIS. CARNEGIE MELLON UNIVERSITY MAKES NO WARRANTIES OF...created in the performance of Federal Government Contract Number FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software

  11. A Taxonomy of Operational Cyber Security Risks Version 2

    DTIC Science & Technology

    2014-05-01

    2014-TN-006 CERT® Division Unlimited distribution subject to the copyright. http://www.sei.cmu.edu Copyright 2014 Carnegie Mellon University...This material is based upon work funded and supported by DHS DoD under Contract No. FA8721-05- C-0003 with Carnegie Mellon University for the...Schilling Circle, Bldg 1305, 3rd floor Hanscom AFB, MA 01731-2125 NO WARRANTY. THIS CARNEGIE MELLON UNIVERSITY AND SOFTWARE ENGINEERING INSTITUTE

  12. DICE: An Object Oriented Programming Environment for Cooperative Engineering Design

    DTIC Science & Technology

    1989-03-20

    environment called PARMENIDES /FRULEKIT; PARMENIDES /FRULEKIT supports programming in frames and rules and was developed in LISP at Carnegie-Mellon...the domain of building design and construction. The Blackboard in DICEY-BUILDER is represented as frames in PARMENIDES , while the KMs are implemented... PARMENIDES fo rart omat format d a b C /envelope BLACKBOAR D machine to machine (’BLACKBOARD l m message f il transfer message p read •d message format J

  13. Agile Software Teams: How They Engage with Systems Engineering on DoD Acquisition Programs

    DTIC Science & Technology

    2014-07-01

    under Contract No. FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software Engineer- ing Institute, a federally funded...issues that would preclude or limit the use of Agile methods within the DoD” [Broadus 2013]. As operational tempos increase and programs fight to...environment in which it operates . This makes software different from other disciplines that have toleranc- es, generally resulting in software engineering

  14. STScI-PRC96-21b DISTANCE MEASUREMENTS TO A TYPE-IA SUPERNOVA BEARING GALAXY

    NASA Technical Reports Server (NTRS)

    2002-01-01

    This Hubble Space Telescope image shows NGC 4639, a spiral galaxy located 78 million light-years away in the Virgo cluster of galaxies. The blue dots in the galaxy's outlying regions indicate the presence of young stars. Among them are young, bright stars called Cepheids, which are used as reliable milepost markers to obtain accurate distances to nearby galaxies. Astronomers measure the brightness of Cepheids to calculate the distance to a galaxy. Allan Sandage's team used Cepheids to measure the distance to NGC 4639, the farthest galaxy to which Cepheid distance has been calculated. After using Cepheids to calculate the distance to NGC 4639, the team compared the results to the peak brightness measurements of SN 1990N, a type Ia supernova located in the galaxy. Then they compared those numbers with the peak brightness of supernovae similarly calibrated in nearby galaxies. The team then determined that type Ia supernovae are reliable secondary distance markers, and can be used to determine distances to galaxies several hundred times farther away than Cepheids. An accurate value for the Hubble Constant depends on Cepheids and secondary distance methods. The color image was made from separate exposures taken in the visible and near-infrared regions of the spectrum with the Wide Field Planetary Camera 2. Credit: A. Sandage (Carnegie Observatories), A. Saha (Space Telescope Science Institute), G.A. Tammann, and L. Labhardt (Astronomical Institute, University Basel), F.D. Macchetto and N. Panagia (Space Telescope Science Institute/ European Space Agency), and NASA Image files in GIF and JPEG format and captions may be accessed on Internet via anonymous ftp from oposite.stsci.edu in /pubinfo.

  15. Demonstrating Diversity in Star-formation Histories with the CSI Survey

    NASA Astrophysics Data System (ADS)

    Dressler, Alan; Kelson, Daniel D.; Abramson, Louis E.; Gladders, Michael D.; Oemler, Augustus, Jr.; Poggianti, Bianca M.; Mulchaey, John S.; Vulcani, Benedetta; Shectman, Stephen A.; Williams, Rik J.; McCarthy, Patrick J.

    2016-12-01

    We present coarse but robust star-formation histories (SFHs) derived from spectrophotometric data of the Carnegie-Spitzer-IMACS Survey, for 22,494 galaxies at 0.3\\lt z\\lt 0.9 with stellar masses of 109 M ⊙ to 1012 M ⊙. Our study moves beyond “average” SFHs and distribution functions of specific star-formation rates (sSFRs) to individually measured SFHs for tens of thousands of galaxies. By comparing star-formation rates (SFRs) with timescales of {10}10,{10}9, and 108 years, we find a wide diversity of SFHs: “old galaxies” that formed most or all of their stars early, galaxies that formed stars with declining or constant SFRs over a Hubble time, and genuinely “young galaxies” that formed most of their stars since z = 1. This sequence is one of decreasing stellar mass, but remarkably, each type is found over a mass range of a factor of 10. Conversely, galaxies at any given mass follow a wide range of SFHs, leading us to conclude that (1) halo mass does not uniquely determine SFHs, (2) there is no “typical” evolutionary track, and (3) “abundance matching” has limitations as a tool for inferring physics. Our observations imply that SFHs are set at an early epoch, and that—for most galaxies—the decline and cessation of star formation occurs over a Hubble time, without distinct “quenching” events. SFH diversity is inconsistent with models where galaxy mass, at any given epoch, grows simply along relations between SFR and stellar mass, but is consistent with a two-parameter lognormal form, lending credence to this model from a new and independent perspective. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.

  16. Emerging Technologies for Software-Reliant Systems

    DTIC Science & Technology

    2011-02-24

    needs • Loose coupling • Global distribution of hardware, software and people • Horizontal integration and convergence • Virtualization...Webinar– February 2011 © 2011 Carnegie Mellon University Global Distribution of Hardware, Software and People Globalization is an essential part of...University Required Software Engineering Emphasis Due to Emerging Technologies (2) Defensive Programming • Security • Auto-adaptation • Globalization

  17. Reading Is a BLAST! Inside an Innovative Literacy Collaboration between Public Schools and the Public Library

    ERIC Educational Resources Information Center

    Genest, Maria T.

    2014-01-01

    Public libraries have long supported the literacy goals of public schools in their communities by providing access to printed and electronic resources that enhance learning and teaching. This article describes an ongoing collaboration between the Carnegie Library of Pittsburgh's BLAST outreach program and the Pittsburgh Public Schools that has…

  18. Faculty Members' Responses to Implementing Re-Envisioned EdD Programs

    ERIC Educational Resources Information Center

    Buss, Ray R.; Zambo, Ron; Zambo, Debby; Perry, Jill A.; Williams, Tiffany R.

    2017-01-01

    Limitations of the education doctorate (EdD) and the emergence of professional practice doctorates have influenced those offering the EdD to re-envision, re-define, and reclaim the EdD as the degree of choice for the next generation of educational leaders. Colleges of education faculty members have used the Carnegie Project on the Education…

  19. Speech to the National Forum on Excellence in Education (Indianapolis, IN, December 6-8, 1983).

    ERIC Educational Resources Information Center

    Simmons, Adele

    Both the Carnegie Report and the Paideia Report argue that all students should study the same curriculum and that significant qualitative change in educational programs is needed. Ernest Boyer's book, "High School," provides evidence of the diversity of the public schools, challenges stereotypes, and suggests that many needed changes can be…

  20. THE ENGLISH PROGRAM OF THE USOE CURRICULUM STUDY AND DEMONSTRATION CENTER MATERIALS CURRENTLY AVAILABLE.

    ERIC Educational Resources Information Center

    1967

    AFTER FIVE YEARS OF FEDERALLY-SUPPORTED CURRICULUM RESEARCH IN ENGLISH, 14 STUDY CENTERS AND FIVE DEMONSTRATION CENTERS ARE NOW MAKING THE RESULTS OF THEIR WORK AVAILABLE TO THE PUBLIC. THIS PAMPHLET LISTS TITLES OF REPORTS AND INSTRUCTIONAL MATERIALS PREPARED BY THE FOLLOWING CENTERS--(1) CARNEGIE-MELLON UNIVERSITY, (2) TEACHERS COLLEGE, COLUMBIA…

  1. Student Perceptions of Digital Story Telling as a Learning-Tool for Educational Leaders

    ERIC Educational Resources Information Center

    LaFrance, Jason; Blizzard, Jason

    2013-01-01

    A study regarding students' perceptions of digital storytelling as a learning tool was conducted in the fall of 2012. The population consisted of 12 students participating in an Administrative Theory course as part of their doctoral program in K-12 or higher education administration at a Carnegie Doctoral Research University in Georgia. During the…

  2. An Analysis of Public Art on University Campuses: Policies, Procedures, and Best Practices

    ERIC Educational Resources Information Center

    Grenier, Michael Robert

    2009-01-01

    This study investigated the policies, procedures, and practices of public art programs on the campuses of research institutions with very high activity as defined by the Carnegie Classification. From this particular type of institution, 55 of the 96 public art administrators provided their opinions, attitudes, and behaviors as part of the "Public…

  3. The Role of Human Intelligence in Computer-Based Intelligent Tutoring Systems.

    ERIC Educational Resources Information Center

    Epstein, Kenneth; Hillegeist, Eleanor

    An Intelligent Tutoring System (ITS) consists of an expert problem-solving program in a subject domain, a tutoring model capable of remediation or primary instruction, and an assessment model that monitors student understanding. The Geometry Proof Tutor (GPT) is an ITS which was developed at Carnegie Mellon University and field tested in the…

  4. Social Science Elective Packages: An Independent Study Program for Grade 12.

    ERIC Educational Resources Information Center

    Moody, David B.

    During the winter semester of 1970 a seminar was conducted for doctoral students in social studies education as a practicum in curriculum development to meet some of the special needs of the small high school, specifically the production of social science independent study packages. The packages produced were one-half Carnegie unit equivalent…

  5. Experimental Effects of Word Generation on Reading Performance in High Poverty Middle Schools

    ERIC Educational Resources Information Center

    Jones, Stephanie M.; Kim, James; LaRusso, Maria; Kim, Ha Yeon; Snow, Catherine

    2015-01-01

    "Time to Act," a 2009 report of the Carnegie Corporation's Council on Advancing Adolescent Literacy, concludes that U.S. students are ill-prepared for the literacy challenges of 21st century higher education, employment, and citizenship. Word Generation (WG) is a research-based vocabulary program for middle school students designed to…

  6. Topological Privacy: Lattice Structures and Information Bubbles for Inference and Obfuscation

    DTIC Science & Technology

    2016-12-19

    AFRL-AFOSR-VA-TR-2017-0036 Topological Privacy Michael Erdmann CARNEGIE MELLON UNIVERSITY 5000 FORBES AVENUE PITTSBURGH, PA 15213-3815 02/22/2017...PERSON 19b. TELEPHONE NUMBER (Include area code) 19-12-2016 Final 15-10-2013 - 14-10-2016 Topological Privacy Erdmann, Michael, A. Carnegie Mellon...Michael Erdmann Carnegie Mellon University me@cs.cmu.edu December 19, 2016 Abstract Information has intrinsic geometric and topological structure, arising

  7. Unique Approach to Threat Analysis Mapping: A Malware Centric Methodology for Better Understanding the Adversary Landscape

    DTIC Science & Technology

    2016-04-05

    Unlimited http://www.sei.cmu.edu CMU/SEI-2016-TR-004 | SOFTWARE ENGINEERING INSTITUTE | CARNEGIE MELLON UNIVERSITY Distribution Statement A...Approved for Public Release; Distribution is Unlimited Copyright 2016 Carnegie Mellon University

 This material is based upon work funded and supported...by Department of Homeland Security under Contract No. FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software

  8. Report Writer and Security Requirements Finder: User and Admin Manuals

    DTIC Science & Technology

    2016-06-15

    Release; Distribution is Unlimited http://www.sei.cmu.edu Copyright 2016 Carnegie Mellon University This material is based upon work funded...and supported by the Department of Defense under Contract No. FA8721-05-C-0003 with Carnegie Mellon University for the operation of the Software...for the SEI Administrative Agent AFLCMC/PZM 20 Schilling Circle, Bldg. 1305, 3rd floor Hanscom AFB, MA 01731-2125 NO WARRANTY. THIS CARNEGIE

  9. Interactive Astronomy.

    ERIC Educational Resources Information Center

    Martin, Jean K.

    1997-01-01

    Presents guiding principles for developing interactive lessons for the World Wide Web. Describes "Amazing Space: Education Online from the Hubble Space Telescope", a program where students study spectacular Hubble Space Telescope images of stars and star-forming regions to learn about the life cycle of stars and the creation of atoms. (JRH)

  10. The Carnegie–Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch

    NASA Astrophysics Data System (ADS)

    Jang, In Sung; Hatt, Dylan; Beaton, Rachael L.; Lee, Myung Gyoon; Freedman, Wendy L.; Madore, Barry F.; Hoyt, Taylor J.; Monson, Andrew J.; Rich, Jeffrey A.; Scowcroft, Victoria; Seibert, Mark

    2018-01-01

    The Carnegie–Chicago Hubble Program (CCHP) seeks to anchor the distance scale of Type Ia supernovae via the Tip of the Red Giant Branch (TRGB) method. Based on deep Hubble Space Telescope ACS/WFC imaging, we present an analysis of the TRGB for the metal-poor halo of NGC 1365, a giant spiral galaxy in the Fornax cluster that was host to the Type Ia supernova SN 2012fr. We have measured the extinction-corrected TRGB magnitude of NGC 1365 to be F814W = 27.34 ± 0.03stat ± 0.04sys mag. In advance of future direct calibration by Gaia, we adopt a provisional I-band TRGB luminosity set at the Large Magellanic Cloud and find a true distance modulus μ 0 = 31.29 ± 0.04stat ± 0.06sys mag or D = 18.1 ± 0.3stat ± 0.5sys Mpc. This measurement is in excellent agreement with recent Cepheid-based distances to NGC 1365 and reveals no significant difference in the distances derived from stars of Populations I and II for this galaxy. We revisit the error budget for the CCHP path to the Hubble constant based on the analysis presented here, i.e., that for one of the most distant Type Ia supernova hosts within our Program, and find that a 2.5% measurement is feasible with the current sample of galaxies and TRGB absolute calibration. Based in part on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #13691.

  11. Using the Feature Exchange Language in the Next Generation Controller

    DTIC Science & Technology

    1990-08-01

    IFCTE DEC 28 The Robotics InstituteCarnegie Mellon University Pittsburgh, PA 15213 LI 4 August 1990 Copyright 0 1990 Carnegie Mellon University The work...ORGANIZATION NAME(S) AND ADDRESS(ES) 8. PERFORMING ORGANIZATION REPORT NUMBER The Robotics Institute Carnegie Mellon University CMU-RI-TR-90-19 Pittsburgh, PA...Basic Syntax 3.1.1. The Grammar The design of FEL syntax is based on a few simple concepts: (1) sentences, (2) verbs, (3) attributes with associated

  12. Chandra X-ray Center

    Science.gov Websites

    NHFP/Einstein Postdoctoral Fellows Selected NASA has announced the selection of the 2018 NASA Hubble . NASA press release Read the full CXC announcement here. 4/3/2018 Accretion in Stellar Systems August 8 Calibration Database User Community Chandra Users' Committee (CUC) NASA Hubble Fellowship Program

  13. Appendange deployment mechanism for the Hubble Space Telescope program

    NASA Technical Reports Server (NTRS)

    Greenfield, H. T.

    1985-01-01

    The key requirements, a design overview, development testing (qualification levels), and two problems and their solutions resolved during the mechanism development testing phase are presented. The mechanism described herein has demonstrated its capability to deploy/restow two large Hubble Space Telescope deployable appendages in a varying but controlled manner.

  14. Rationale for a ’Many Maps’ Phonology Machine

    DTIC Science & Technology

    1990-03-01

    City, State, and ZIP Code) 10 SOURCE OF FUNDING NUMBERS 40005ub201/7-4-86 PROGRAM PROJECT TASK ~ WORK UNIT ELEMENT NO NO.I NO. ACCESSION NO NIA N/A NIA...seek to verify or refute. Some day, neurolinguistics may provide the decisive answer to the rationalist/empiricist debate. If so, we are confident that...linguistics program , Carnegie Mellon University. [7] Touretzky, D. S. (1989) Toward a connectionist phonology: the "many maps" ap- proach to sequencc

  15. Brief History of Computer-Assisted Instruction at the Institute for Mathematical Studies in the Social Sciences.

    ERIC Educational Resources Information Center

    Stanford Univ., CA. Inst. for Mathematical Studies in Social Science.

    In 1963, the Institute began a program of research and development in computer-assisted instruction (CAI). Their efforts have been funded at various times by the Carnegie Corporation of New York, The National Science Foundation and the United States Office of Education. Starting with a medium-sized computer and six student stations, the Institute…

  16. Research Becomes You: Cultivating EdD Students' Identities as Educational Leaders and Researchers and a "Learning by Doing" Meta-Study

    ERIC Educational Resources Information Center

    Buss, Ray R.; Avery, Andrea

    2017-01-01

    We examined how end-of-first-year students in a Carnegie Project on the Education Doctorate (CPED)-affiliated EdD program were developing professional identities as educational leaders and researchers. Quantitative and qualitative data revealed substantial development of leadership skills, but even greater growth in perceptions of research skills.…

  17. Turning Points: States in Action. An Interim Report of the Middle Grade School State Policy Initiative.

    ERIC Educational Resources Information Center

    Council of Chief State School Officers, Washington, DC. Resource Center on Educational Equity.

    This report analyzes the experiences of 27 states selected to participate in Carnegie Corporation of New York's Middle Grade School State Policy Initiative (MGSSPI), a 3-year grant program to states to stimulate fundamental reform in schools serving 10- to 15-year old students. MGSSPI states are working to radically transform the education…

  18. A Qualitative Study of the Curricula for the Doctor of Education (EdD) Degree in Higher Education Programs

    ERIC Educational Resources Information Center

    Holland, Rebecca C.

    2017-01-01

    Using the Carnegie Project for the Education Doctorate (CPED) as a model curricular framework, this study sought to determine the structures and functions of well-run and respected non-CPED participating higher education administration EdD curricula. The qualitative approach was used during two iterations of focus groups to learn the professional…

  19. Comparative Effectiveness of Carnegie Learning's "Cognitive Tutor" Algebra I Curriculum: A Report of a Randomized Experiment in the Maui School District. Research Report

    ERIC Educational Resources Information Center

    Cabalo, Jessica Villaruz; Vu, Minh-Thien

    2007-01-01

    The Maui Hawaii Educational consortium (the Maui School District and Maui Community College) sought scientifically based evidence for the effectiveness of the "Cognitive Tutor (CT) Algebra I Curriculum" to inform adoption decisions. Decision makers were particularly interested in whether the use of the "CT" program affects…

  20. Emerging Software Development and Acquisition Approaches: Panacea or Villain

    DTIC Science & Technology

    2011-05-16

    2010 Carnegie Mellon University Emerging Software Development and Acquisition Approaches: Panacea or Villain Software Engineering Institute...aspect of this collection of information, including suggestions for reducing this burden, to Washington Headquarters Services , Directorate for...Emerging Software Development and Acquisition Approaches: Panacea or Villain 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S

  1. Use of Learner-Centered Strategies in the Preparation of Community and Technical College Leaders: Assessments by Participating Doctoral Students

    ERIC Educational Resources Information Center

    Browne-Ferrigno, Tricia; Muth, Rodney

    2010-01-01

    This paper presents assessments by students actively engaged in a recently redesigned Doctor of Education (EdD) program, delivered at a research-extensive university participating in the the Carnegie Project on the Education Doctorate (CPED), to prepare leaders for a statewide system of community and technical colleges. Because a unique feature of…

  2. Mothers of Invention: Hubble Engineers Push Robotic 'Evolution' to Save Telescope, Enable New Exploration

    NASA Technical Reports Server (NTRS)

    Morring, Frank, Jr.

    2004-01-01

    Robotic technology being developed out of necessity to keep the Hubble Space Telescope operating could also lead to new levels of man-machine team-work in deep-space exploration down the road-if it survives the near-term scramble for funding. Engineers here who have devoted their NASA careers to the concept of humans servicing the telescope in orbit are planning modifications to International Space Station (ISS) robots that would leave the humans on the ground. The work. forced by post-Columbia flight rules that killed a planned shuttle-servicing mission to Hubble, marks another step in the evolution of robot-partners for human space explorers. "Hubble has always been a pathfider for this agency," says Mike Weiss. Hubble deputy program manager technical. "When the space station was flown and assembled, Hubble was the pathfinder. not just for modularity, but for operations, for assembly techniques. Exploration is the next step. Things we're going to do on Hubble are going to be applied to exploration. It's not just putting a robot in space. It's operating a robot in space. It's adapting that robot to what needs to be done the next time you're up there."

  3. The Carnegie Observatories

    Science.gov Websites

    , Receives Prestigious Goldwater Scholarship 2018 Astronomy Lecture Series Are You Rocky or are You Gassy - 4:00pm TBD Colloquium by Dr. Alan Dressler (Carnegie) Astronomy Lecture Series Online You can now

  4. An innovation in physician training: the Clinical Scholars Program.

    PubMed

    Shuster, A L; Cluff, L E; Haynes, M A; Hook, E W; Rogers, D E

    1983-02-01

    The Robert Wood Johnson Foundation Clinical Scholars Program was developed to allow selected physician clinicians to acquire certain skills which are not part of the usual physician's repertoire. Begun in 1969 with support from the Carnegie Corporation and the Commonwealth Fund, funding has been provided since 1973 by the Robert Wood Johnson Foundation. By June 1981, 309 physicians had completed their training as clinical scholars, and a majority were pursuing careers in academic medicine. This paper recounts the factors and forces which led to the initiation and development of the program, its successes and failures, the problems faced, the achievements of clinical scholar alumni, and the program's current status.

  5. Modeling the Evolution of a Science Project in Software-Reliant System Acquisition Programs

    DTIC Science & Technology

    2013-07-24

    might: • Limit worker burnout • Perform better regarding schedule 10 Software Technology Conference April 10, 2013 © 2013 Carnegie Mellon...University The Evolution of a Science Project Key Preliminary Findings -3 The tipping point contributes to the “90% Done” Syndrome Percentage...worker burnout - SP User Satisfaction SP increasing satisfaction indicated satisfaction + + B3 Moderating User Satisfaction overage switch demand switch

  6. Brain Imaging and rTMS Studies of Individual Differences in Cognitive Processing

    DTIC Science & Technology

    2013-08-09

    Institution: Address: Phone: Fax: Email : Web Page: Contract: Project Title: Program Officer: Dr. Marcel Adam Just Carnegie Mellon University...and multitasking ) are included in the progress report using well established sets of materials. In the sentence and discourse tasks, participants...compensatory partnerships and the re-emergence of the primary regions. 3. Cortical reorganization induced by rTMS during multitasking (listening to

  7. A Taxonomy of Operational Risks

    DTIC Science & Technology

    2005-09-01

    the operational organization. Con - tractual constraints or requirements can impose risk if the mission delivers products or services under contract...Carnegie Mellon Software Engineering Institute A Taxonomy of Operational Risks CMU/SEI-2005-TN-036 Brian P. Gallagher Pamela J. Case DIST...Operational Risks CMU/SEI-2005-TN-036 Brian P. Gallagher Pamela J. Case Rita C. Creel Susan Kushner Ray C. Williams September2005 Acquisition Support Program

  8. SEPG Europe 2012 Conference Proceedings

    DTIC Science & Technology

    2012-09-01

    Process Management http://www.sei.cmu.edu SEI markings v3.2/ DM-0000022 / 30 August 2011 Copyright 2012 Carnegie Mellon University This material...Change Management Decisions in Large Enterprise Transformation Programs 18 3.1 Abstract 18 3.2 Introduction 18 3.3 Barriers for Transformation 18...Case Study #3: Enterprise Transformation Through Enterprise Data Management (Investment and Asset Management ) 25 3.7 Conclusions and Recommendations 27

  9. Architectural Implications of Cloud Computing

    DTIC Science & Technology

    2011-10-24

    Public Cloud Infrastructure-as-a- Service (IaaS) Software -as-a- Service ( SaaS ) Cloud Computing Types Platform-as-a- Service (PaaS) Based on Type of...Twitter #SEIVirtualForum © 2011 Carnegie Mellon University Software -as-a- Service ( SaaS ) Model of software deployment in which a third-party...and System Solutions (RTSS) Program. Her current interests and projects are in service -oriented architecture (SOA), cloud computing, and context

  10. Pelagic erosion and sedimentation north of Carnegie Ridge, eastern equatorial Pacific

    NASA Astrophysics Data System (ADS)

    Brooks, C. K.; Lyle, M. W.; Marcantonio, F.; Lewis, D. M.; Paul, C.

    2011-12-01

    The Carnegie Ridge is one of three bathymetric highs bounding the Panama Basin and is known to exhibit erosion and redeposition of pelagic sediments. The extent of erosion and redeposition was studied during the R/V Melville cruise MV1014 in November 2010 to compare with geochemical estimates of sediment focusing. The MV1014 cruise acquired geochemical, geological and geophysical data using multichannel 2-D seismic and 3.5 kHz sub-bottom profiler, swathmap bathymetry, coring, and water casts. The seismic reflection, digital sub-bottom profiler and swathmap bathymetry data were used to investigate biogenic sedimentary deposition in the Panama Basin and erosion from Carnegie Ridge. We compare the new geophysical results with drilling on ODP Leg 202, the NEMO-03 site survey cruise for Leg 202, an early survey from 1969 and other data compiled by Ecuadorian surveys. Areas of non-deposition and/or erosion include the bathymetric highs along the ridge, seamounts, and an area of interest, a valley located on the northwestern flank of the ridge. The valley encompasses 183 km2 and exhibits large scale erosion, cutting down through sediments deposited over the 10-million year life of this segment of the Carnegie Ridge. All other valleys located within the Carnegie Ridge study area demonstrate ample deposition with sedimentary packages ranging from 200-800m with an average value trending around 400m. Higher sediment deposition is found in basins to the north of the erosional valley but similar sedimentation is also found even further north, beyond intervening high topography. The thickest sediment deposit near the Carnegie Ridge is actually found on the southern flank of the ridge, more than 100 km to the south of the survey area. Digital chirp sub-bottom profiler data combined with high-resolution seismic illustrate changes in sedimentation and erosion on the Carnegie Ridge, highlighting the dynamic sedimentary environment.

  11. "Amazing Space": Creating Educational Resources from Current Scientific Research Results from the Hubble Space Telescope.

    ERIC Educational Resources Information Center

    Christian, C. A.; Eisenhamer, B.; Eisenhamer, Jonathan; Teays, Terry

    2001-01-01

    Introduces the Amazing Space program which is designed to enhance student mathematics, science, and technology skills using recent data and results from the National Aeronautics and Space Administration's (NASA) Hubble Space Telescope mission. Explains the process of designing multi-media resources in a five-week summer workshop that partners…

  12. Extravehicular Activity Probabilistic Risk Assessment Overview for Thermal Protection System Repair on the Hubble Space Telescope Servicing Mission

    NASA Technical Reports Server (NTRS)

    Bigler, Mark; Canga, Michael A.; Duncan, Gary

    2010-01-01

    The Shuttle Program initiated an Extravehicular Activity (EVA) Probabilistic Risk Assessment (PRA) to assess the risks associated with performing a Shuttle Thermal Protection System (TPS) repair during the Space Transportation System (STS)-125 Hubble repair mission as part of risk trades between TPS repair and crew rescue.

  13. VizieR Online Data Catalog: >20yrs of HST obs. of Cepheids in SNIa host gal. (Hoffmann+, 2016)

    NASA Astrophysics Data System (ADS)

    Hoffmann, S. L.; Macri, L. M.; Riess, A. G.; Yuan, W.; Casertano, S.; Foley, R. J.; Filippenko, A. V.; Tucker, B. E.; Chornock, R.; Silverman, J. M.; Welch, D. L.; Goobar, A.; Amanullah, R.

    2017-01-01

    HST observations of Cepheid variables (both archival or newly obtained) span more than two decades (1994-2016; see table 1). The earliest Cepheid observations we analyzed were obtained with the Wide Field and Planetary Camera 2 (WFPC2) as part of the initial efforts to measure H0 with HST (Freedman+ 2001ApJ...553...47F; Sandage+ 2006ApJ...653..843S) and were later used by Freedman+ (2012ApJ...758...24F) to reach beyond the LMC for the Carnegie Hubble Project. We also re-analyzed observations obtained in previous phases of our project (Riess+ 2009, J/ApJS/183/109; 2011, J/ApJ/730/119) with the Advanced Camera for Surveys (ACS) Wide Field Channel (WFC) and/or the Wide Field Camera 3 (WFC3) Ultraviolet and Visible Channel (UVIS). Finally, we obtained new observations of nine SN Ia hosts using WFC3. We obtained the majority of our optical images with these modern cameras, 113 and 132 unique epochs with ACS and WFC3, respectively, while WFPC2 contributes a smaller fraction with 67 epochs. (6 data files).

  14. Change Strategies Used by a Proprietary School: The Dale Carnegie Organization.

    ERIC Educational Resources Information Center

    Mackey, Paul J.

    1983-01-01

    Discusses recent developments regarding proprietary schools: recognition by accrediting associations, increased federal aid, and increased need for the specific training offered by these schools. Uses the Dale Carnegie organization as an example. (JOW)

  15. 77 FR 43337 - Drugs for Human Use; Drug Efficacy Study Implementation; Certain Prescription Drugs Offered for...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-07-24

    .... (now part of Kremers-Urban Pharmaceuticals, Inc., 902 Carnegie Center, Suite 360, Princeton, NJ 08540...-687) and Spasmolin (ANDA 86-655); Sandoz, Inc., 506 Carnegie Center, Suite 400, Princeton, NJ 08540...

  16. Computer Science Research Review 1974-75

    DTIC Science & Technology

    1975-08-01

    mwmmmimmm^m^mmmrm. : i i 1 Faculty and Visitors Mario Barbaccl Research Associate B.S., Universidad Nacional de Ingenieria , Lima, Peru (1966...Engineer, Universidad Nacional de Ingenieria , Lima, Peru (1968) Ph.D., Carnegie-Mellon University (1974) Carnegie. 1969: Design Automation

  17. Hubble space telescope: The GO and GTO observing programs, version 3.0

    NASA Technical Reports Server (NTRS)

    Downes, Ron

    1992-01-01

    A portion of the observing time with the Hubble Space Telescope (HST) was awarded by NASA to scientists involved in the development of the HST and its instruments. These scientists are the Guaranteed Time Observers (GTO's). Observing time was also awarded to General Observers (GO's) on the basis of the proposal reviews in 1989 and 1991. The majority of the 1989 programs have been completed during 'Cycle 1', while the 1991 programs will be completed during 'Cycle 2', nominally a 12-month period beginning July 1992. This document presents abstracts of these GO and GTO programs, and detailed listings of the specific targets and exposures contained in them. These programs and exposures are protected by NASA policy, as detailed in the HST Call for Proposals (CP), and are not to be duplicated by new programs.

  18. Certified Binaries for Software Components

    DTIC Science & Technology

    2007-09-01

    is sponsored by the U.S. Department of Defense. The Software Engineering Institute is a federally funded research and development center sponsored...by the U.S. Department of Defense. Copyright 2007 Carnegie Mellon University. NO WARRANTY THIS CARNEGIE MELLON UNIVERSITY AND SOFTWARE ENGINEERING

  19. Island emergence/subsidence histories and their bearing upon biological speciation in the Galápagos

    NASA Astrophysics Data System (ADS)

    Orellana Rovirosa, F.

    2017-12-01

    In the context of plate motion reconstructions for the Nazca, Cocos and South American plates in relation with the Galápagos hotspot, it is found that the age-depth dependence of bathymetry, dynamic topography due to the Galápagos plume, crustal relaxation, and magmatic production allow for us to estimate the subsidence of islands and seamounts along the Carnegie Ridge. Our estimates are partially based on geodynamic theory (fluid mechanics and elasticity), but also on detailed bathymetric observations and analysis. For the Carnegie Ridge saddle, we estimate subsidence of about 2 km occurring during the past 13 Ma. Because the present-day depths of the region are in the range 2-2.5 km, this assessment shows that the deepest region of the present-day Carnegie Ridge may have been above sea level when it was closer to the active hotspot, therefore providing habitat for land species for a few (<5) million years. Moreover, the migrating hotspot swell may have caused the emerging of different portions of the Carnegie Ridge on a spatio-temporal progression. A more sophisticated 3D numerical model including an asthenosphere and plume interacting with the overlying Nazca plate may provide an improved understanding of geological-biological co-evolution in the Galápagos-Carnegie Ridge.

  20. Are Case Studies a Good Teaching Tool for CS1?

    DTIC Science & Technology

    1995-01-01

    old AP/CS tests to compare our students’ performance against the results obtained by ETS. Currently, the introductory courses at CMU are taught using...Carrasquel, J., Goldenson, D. & Miller, P. L. (1985). Competency Testing in Introductory Computer Science: The Mastery Examination at Carnegie Mellon... courses is that many places do not have enough facilities (or the necessary time) required for long programming assignments. In our opinion, using case

  1. Astronaut Anna Fisher in NBS Training For Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher training on a mock-up of a modular section of the HST for an axial scientific instrument change out.

  2. Neutral Buoyancy Test - Hubble Space Telescope Scientific Instruments (SI)

    NASA Technical Reports Server (NTRS)

    1979-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the first and flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Pictured is MSFC's Neutral Buoyancy Simulator that served as the test center for shuttle astronauts training for Hubble related missions. Shown is an astronaut training on a mock-up of a modular section of the HST in the removal and replacement of scientific instruments.

  3. Detection of Sources of Harmful Radiation using Portable Sensors

    DTIC Science & Technology

    2016-05-01

    Department Carnegie Mellon University Pittsburgh, PA Thesis Committee Artur Dubrawski, Chair Srinivas Narasimhan Submitted in partial fulfillment of the...Aggregation of Evidence for Detection and Characterization of Patterns in Multiple Noisy Observations”. PhD thesis. Carnegie Mellon, 2015. [15] Prateek Tandon

  4. Laterally Vibrating Resonator Based Elasto-Optic Modulation in Aluminum Nitride

    DTIC Science & Technology

    2016-08-15

    Department of Electrical and Computer Engineering, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA (Received 1 February 2016; accepted...to acknowledge process related support from the staff at the Carnegie Mellon Nanofabrication Facility as well as funding support from the National

  5. Leveraging Relational Technology through Industry Partnerships.

    ERIC Educational Resources Information Center

    Brush, Leonard M.; Schaller, Anthony J.

    1988-01-01

    Carnegie Mellon University has leveraged its technological expertise with database management systems (DBMS) into joint technological and developmental partnerships with DBMS and application software vendors. Carnegie's relational database strategy, the strategy of partnerships and how they were formed, and how the partnerships are doing are…

  6. A Magnified View of the Epoch of Reionization with the Hubble Frontier Fields

    NASA Astrophysics Data System (ADS)

    Livermore, Rachael C.; Finkelstein, Steven L.; Lotz, Jennifer M.

    2017-06-01

    The Hubble Frontier Fields program has obtained deep optical and near-infrared Hubble Space Telescope imaging of six galaxy clusters and associated parallel fields. The depth of the imaging (m_AB ~ 29) means we can identify faint galaxies at z >6, and those in the cluster fields also benefit from magnification due to strong gravitational lensing. Using wavelet decomposition to subtract the foreground cluster galaxies, we can reach intrinsic absolute magnitudes of M_UV ~ -12.5 at z ~ 6. Here, we present the UV luminosity functions at 6

  7. The UV Luminosity Function at 6 < z < 10 from the Hubble Frontier Fields

    NASA Astrophysics Data System (ADS)

    Livermore, Rachael C.; Finkelstein, Steven L.; Lotz, Jennifer M.

    2017-01-01

    The Hubble Frontier Fields program has obtained deep optical and near-infrared Hubble Space Telescope imaging of six galaxy clusters and associated parallel fields. The depth of the imaging (m_AB ~ 29) means we can identify faint galaxies at z > 6, and those in the cluster fields also benefit from magnification due to strong gravitational lensing that allows us to reach intrinsic absolute magnitudes of M_UV ~ -12.5 at z ~ 6. Here, we present the UV luminosity functions at 6 < z < 10 from the complete Hubble Frontier Fields data, revealing a steep faint-end slope that extends to the limits of the data. The lack of any apparent turnover in the luminosity functions means that faint galaxies in the early Universe may have provided sufficient ionizing radiation to sustain reionization.

  8. KSC-02pd0627

    NASA Image and Video Library

    2002-04-30

    KENNEDY SPACE CENTER, FLA. -- At the 2002 Space Congress, Cape Canaveral, Fla., a presentation on "Hubble Discoveries" by Dr. Mark Clampin (with microphone), Advanced Camera for Surveys team, included an image of an eye (seen on the screen) comprising hundreds of photos of all the people who worked on Hubble. On the right is Frank Ceppolina, project manager, Hubble Space Telescope Development Project. The Space Congress is held annually to highlight military and space initiatives, new technologies, and Florida's role in programs and research. This year's theme is Beginning a New Era - Initiatives in Space. NASA presented several paper sessions, including Advancements in Technology. Space Congress is sponsored by the Canaveral Council of Technical Societies

  9. Report of the President.

    ERIC Educational Resources Information Center

    Gregorian, Vartan

    The occasion of the anniversary of Andrew Carnegie's transfer of wealth from business to philanthropy provides an opportunity to reflect on Carnegie's role in philanthropy and philanthropy's role, responsibilities, and challenges in the nation. Citizen philanthropy has been an important constituent of participatory democracy in the United States,…

  10. Change as a Constant: Organizational Restructuring at Carnegie Mellon University.

    ERIC Educational Resources Information Center

    Keating, Patrick J.; And Others

    1996-01-01

    The origins and strategies for change in the administrative structure of Carnegie Mellon University (Pennsylvania) are discussed, including trends within all of higher education and conditions specific to the university. Quality improvement efforts are described briefly. Special attention is given to the institution's procurement-disbursement…

  11. Quasars and the Caltech-Carnegie Connection

    NASA Astrophysics Data System (ADS)

    Waluska, Edward R.

    2006-12-01

    A collaborative relationship existed between the California Institute of Technology(Caltech) and the Carnegie Institution of Washington (Carnegie) beginning in 1946, when a formal agreement was made between the two groups of trustees. This agreement was designed to integrate Mount Wilson Observatory with the new unfinished Palomar Observatory into a single scientific entity. During the period from 1946 to 1979, much astronomical research was done at both institutions as a direct result of this collaboration. Part of this research included the first identification of a radio source with an apparently stellar object by Allan Sandage of Carnegie and Thomas Matthews of Caltech in 1960, and the first identification of the spectral lines from a radio source associated with such an object by Maarten Schmidt of Caltech in 1963. This paper examines how the discovery of these objects, which came to be known as quasars, and the subsequent research on these objects, impacted the relationship between Caltech and Carnegie, such that the relationship was formally dissolved in 1980. In this paper, the controversy surrounding the discovery and the interpretation of quasars is examined to provide further understanding about the working relationship when the two institutions were formally collaborating. Some of the data used in this paper were drawn from interviews of the researchers themselves, and this research forms part of a dissertation for a PhD degree from James Cook University in Townsville, Australia.

  12. The Process in Completing a Nontraditional Group Dissertation in Practice for the Carnegie Project on the Education Doctorate, the Ed.D. Educational Leadership Program at Lynn University

    ERIC Educational Resources Information Center

    Vickers, Jerome

    2016-01-01

    This study focused on how a cohort of scholarly practitioners extended the traditional Doctorate in Education (Ed.D.) model at Lynn University by undertaking a nontraditional group Dissertation in Practice (DiP). The participants were a cohort of 11 scholarly practitioners known as Cohort 5 who became the first Lynn University doctoral students to…

  13. An Assessment of the Effectiveness of Air Force Risk Management Practices in Program Acquisition Using Survey Instrument Analysis

    DTIC Science & Technology

    2015-06-18

    Engineering Effectiveness Survey. CMU/SEI-2012-SR-009. Carnegie Mellon University. November 2012. Field, Andy. Discovering Statistics Using SPSS , 3rd...enough into the survey to begin answering questions on risk practices. All of the data statistical analysis will be performed using SPSS . Prior to...probabilistically using distributions for likelihood and impact. Statistical methods like Monte Carlo can more comprehensively evaluate the cost and

  14. WebWatcher: Machine Learning and Hypertext

    DTIC Science & Technology

    1995-05-29

    WebWatcher: Machine Learning and Hypertext Thorsten Joachims, Tom Mitchell, Dayne Freitag, and Robert Armstrong School of Computer Science Carnegie...HTML-page about machine learning in which we in- serted a hyperlink to WebWatcher (line 6). The user follows this hyperlink and gets to a page which...AND SUBTITLE WebWatcher: Machine Learning and Hypertext 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT

  15. DoD Information Assurance and Agile: Challenges and Recommendations Gathered Through Interviews with Agile Program Managers and DoD Accreditation Reviewers

    DTIC Science & Technology

    2012-11-01

    Tradeoff Analysis Method; ATAM, Capability Maturity Model , Capability Maturity Modeling , Carnegie Mellon, CERT, CERT Coordination Center, CMM, CMMI...Hermansen, Product Design, Sphere of Influence (https://www.SphereOfInfluence.com) Joel McAteer, Information Assurance Manager, Modeling ...use of them does introduce some challenges related to delivering software features rapidly and/or in- crementally . • Challenges with respect to

  16. Next Steps for the 1980s in Student Financial Aid. A Fourth Alternative. Comments and Recommendations by the Carnegie Council on Policy Studies in Higher Education.

    ERIC Educational Resources Information Center

    Carnegie Council on Policy Studies in Higher Education, Berkeley, CA.

    In 1979 the Congress and the administration will consider legislation to extend and revise the Higher Education Act and, in the process, will review the structure of the student-aid system. Several alternatives are likely to be considered, but a fourth is proposed here: a major overhaul of the existing package of programs to make them more…

  17. 1986 Year End Report for Road Following at Carnegie-Mellon

    DTIC Science & Technology

    1987-05-01

    how to make them work efficiently. We designed a hierarchical structure and a monitor module which manages all parts of the hierarchy (see figure 1...database, called the Local Map, is managed by a program known as the Local Map Builder (LMB). Each module stores and retrieves information in the...knowledge-intensive modules, and a database manager that synchronizes the modules-is characteristic of a traditional blackboard system. Such a system is

  18. Process Guide for the Domain-Specific Software Architectures (DSSA) Process Life Cycle

    DTIC Science & Technology

    1993-12-01

    of box "Things" used and transformed by activities Output Right side of box...Carnegie Mellon University is required not to chsc’lmirate in admission. employment or administration of its programs on the oasis of race. color...natonal Origin sex of hanoicap ,:zlaon of Tit!e VI of.the C~vii RAgtts A - of 964 Tile ’X of ’he Educationai Amendments of 1972 and Sectlon 504 of

  19. The Effect of Relational Database Technology on Administrative Computing at Carnegie Mellon University.

    ERIC Educational Resources Information Center

    Golden, Cynthia; Eisenberger, Dorit

    1990-01-01

    Carnegie Mellon University's decision to standardize its administrative system development efforts on relational database technology and structured query language is discussed and its impact is examined in one of its larger, more widely used applications, the university information system. Advantages, new responsibilities, and challenges of the…

  20. Inspiring Teaching. Carnegie Professors of the Year Speak.

    ERIC Educational Resources Information Center

    Roth, John K., Ed.

    Twenty-one essays describe the successful teaching strategies used by faculty who have been named "Teacher of the Year" by the Carnegie Foundation for the Advancement of Teaching. Essays are grouped into those which focus on: teaching characteristics, teaching practices, teaching philosophies, and teaching teachers. The essays are: (1)…

  1. Carnegie Learning Curricula and Cognitive Tutor[R] Software. What Works Clearinghouse Intervention Report

    ERIC Educational Resources Information Center

    What Works Clearinghouse, 2010

    2010-01-01

    The combination of "Carnegie Learning Curricula and Cognitive Tutor[R] Software" merges algebra textbooks with interactive software developed around an artificial intelligence model that identifies strengths and weaknesses in an individual student's mastery of mathematical concepts. The software customizes prompts to focus on areas in…

  2. Attaining Carnegie's Community-Engagement Classification

    ERIC Educational Resources Information Center

    Zuiches, James J.

    2008-01-01

    Now that the Carnegie Foundation for the Advancement of Teaching has designated a first round of institutions that meet its criteria for engagement with their communities, in this article, the authors offer their reflections on the process for other colleges and universities preparing similar applications. They learned a great deal about their own…

  3. The New Social Studies in Perspective: The Carnegie-Mellon Slow-Learner Project.

    ERIC Educational Resources Information Center

    Penna, Anthony N.

    1995-01-01

    Describes the origins, development, and products of the slow- learner social studies curriculum development project at Carnegie-Mellon University (Pennsylvania) in the late 1960s. Maintains that this project represented the last wave of curriculum projects to emerge from the national reform efforts following Sputnik. (CFR)

  4. A nuclear data approach for the Hubble constant measurements

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Pritychenko, B.

    2015-06-09

    An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP) codes and procedures have been applied to resolve this issue. The nuclear data approach has produced the most probable or recommended Hubble constant value of 67.00(770) (km/sec)/Mpc. This recommended value is based on the last 25 years of experimental research and includes contributions from different types of measurements. The present result implies (14.6±1.7) x 10 9 years as a rough estimate for the age of the Universe. The complete list of recommended results is given and possiblemore » implications are discussed.« less

  5. Hubble Space Telescope Discovery of a Probable Caustic-Crossing Event in the MACS1149 Galaxy Cluster Field

    NASA Astrophysics Data System (ADS)

    Kelly, Patrick L.; Rodney, Steven; Diego, Jose Maria; Zitrin, Adi; Broadhurst, Tom; Selsing, Jonatan; Balestra, Italo; Benito, Alberto Molino; Bradac, Marusa; Bradley, Larry; Brammer, Gabriel; Cenko, Brad; Christensen, Lise; Coe, Dan; Filippenko, Alexei V.; Foley, Ryan; Frye, Brenda; Graham, Melissa; Graur, Or; Grillo, Claudio; Hjorth, Jens; Howell, Andy; Jauzac, Mathilde; Jha, Saurabh; Kaiser, Nick; Kawamata, Ryota; Kneib, Jean-Paul; Lotz, Jennifer; Matheson, Thomas; McCully, Curtis; Merten, Julian; Nonino, Mario; Oguri, Masamune; Richard, Johan; Riess, Adam; Rosati, Piero; Schmidt, Kasper Borello; Sharon, Keren; Smith, Nathan; Strolger, Lou; Treu, Tommaso; Wang, Xin; Weiner, Ben; Williams, Liliya; Zheng, Weikang

    2016-05-01

    While monitoring the MACS1149 (z = 0.54) galaxy cluster as part of the RefsdalRedux program (PID 14199; PI Kelly) with the Hubble Space Telescope (HST) WFC3 IR camera, we have detected a rising transient that appears to be coincident ( Target-of-opportunity optical follow-up imaging in several ACS and WFC3 bands with the FrontierSN program (PID 14208; PI Rodney) has revealed that its rest-frame ultraviolet through optical spectrum may be reasonably well fit with that of a B star at z=1.49 exhibiting a strong Balmer break.

  6. National Study of Excellence and Innovation in Physical Therapist Education: Part 2-A Call to Reform.

    PubMed

    Jensen, Gail M; Hack, Laurita M; Nordstrom, Terrence; Gwyer, Janet; Mostrom, Elizabeth

    2017-09-01

    This perspective shares recommendations that draw from (1) the National Study of Excellence and Innovation in Physical Therapist Education research findings and a conceptual model of excellence in physical therapist education, (2) the Carnegie Foundation's Preparation for the Professions Program (PPP), and (3) research in the learning sciences. The 30 recommendations are linked to the dimensions described in the conceptual model for excellence in physical therapist education: Culture of Excellence, Praxis of Learning, and Organizational Structures and Resources. This perspective proposes a transformative call for reform framed across 3 core categories: (1) creating a culture of excellence, leadership, and partnership, (2) advancing the learning sciences and understanding and enacting the social contract, and (3) implementing organizational imperatives. Similar to the Carnegie studies, this perspective identifies action items (9) that should be initiated immediately in a strategic and systematic way by the major organizational stakeholders in physical therapist education. These recommendations and action items provide a transformative agenda for physical therapist education, and thus the profession, in meeting the changing needs of society through higher levels of excellence. © 2017 American Physical Therapy Association.

  7. The Carnegie Classification of Institutions of Higher Education. 2000 Edition. A Technical Report.

    ERIC Educational Resources Information Center

    Carnegie Foundation for the Advancement of Teaching, Menlo Park, CA.

    The Carnegie Classification of Institutions of Higher Education is the framework in which institutional diversity in United States higher education is commonly described. Developed in 1971, the Classification was designed to support research in higher education by identifying categories of colleges and universities that would be homogeneous with…

  8. CCRIS: Carnegie Commission Reports Information System.

    ERIC Educational Resources Information Center

    Lavin, Mary Jo

    The Carnegie Commission Reports Information System (CCRIS) attempts to make the findings of the 22 Commission reports (published by McGraw Hill Book Company) more readily available to the academic community. CCRIS consists of an explanatory text of 16 pages introducing the reader to a set of 1500 edge-notched McBee cards. Each card contains a…

  9. Pathways Post-Participation Outcomes: Preliminary Findings. Carnegie Math Pathways Research Brief

    ERIC Educational Resources Information Center

    Norman, Jon

    2017-01-01

    The Carnegie Foundation for the Advancement of Teaching's Math Pathways seek to improve outcomes for community college students who take remedial math courses. The Pathways include two comprehensive instructional systems--Statway® and Quantaway® and are described in this report. They are designed to support students to achieve the necessary math…

  10. Carnegie Units and High School Attendance Policies: An Absence of Thought?!?

    ERIC Educational Resources Information Center

    Outhouse, Craig Michael

    2012-01-01

    This case was developed as part of a doctoral course for educational administration students who were specializing in K-12 educational administration. It could be used in a leadership, special education, or policy course for future school leaders or teachers. Currently, most educational institutions use Carnegie Units to structure how students…

  11. Carnegie's New Community Engagement Classification: Affirming Higher Education's Role in Community

    ERIC Educational Resources Information Center

    Driscoll, Amy

    2009-01-01

    In 2005, the Carnegie Foundation for the Advancement of Teaching (CFAT) stirred the higher education world with the announcement of a new classification for institutions that engage with community. The classification, community engagement, is the first in a set of planned classification schemes resulting from the foundation's reexamination of the…

  12. The Carnegie Unit: Past, Present, and Future

    ERIC Educational Resources Information Center

    Silva, Elena; White, Taylor

    2015-01-01

    For more than a century, the Carnegie Unit has been the central organizing feature of American education. Translated into the "credit hour" in higher education (roughly, one hour of class time per week in a 14-16 week semester), this time-based unit is embedded in nearly every aspect of the system, from faculty-workload and…

  13. Creating Women's Work in the Academy and beyond: Carnegie Connections, 1923-1942

    ERIC Educational Resources Information Center

    Collins, Jenny

    2009-01-01

    This paper examines the significance of the Dominion and Colonies Fund under the presidency of Frederick Paul Keppel and details ways in which the Carnegie Corporation worked to internationalize American educational theories and practices. It challenges previous scholarship claims that grants made were largely extensions of the Corporation's…

  14. The Carnegie Project on the Education Doctorate

    ERIC Educational Resources Information Center

    Perry, Jill Alexa

    2015-01-01

    Beginning with 21 US schools of education, the Carnegie Project on the Education Doctorate (CPED) has created a network of education faculty who are differentiating the EdD from the PhD in order to better meet the needs of their practitioner-scholar students. Their discussions center on two questions: "What are the knowledge, skills, and…

  15. Analysis of the Carnegie Classification of Community Engagement: Patterns and Impact on Institutions

    ERIC Educational Resources Information Center

    Driscoll, Amy

    2014-01-01

    This chapter describes the impact that participation in the Carnegie Classification for Community Engagement had on the institutions of higher learning that applied for the classification. This is described in terms of changes in direct community engagement, monitoring and reporting on community engagement, and levels of student and professor…

  16. A Database Architecture for Web-Based Distance Education.

    ERIC Educational Resources Information Center

    Rehak, Daniel R.

    The goal of the Carnegie Mellon Online project is to build an infrastructure for delivery of courses via the World Wide Web. The project aims to deliver educational content and to assess student competency in support of courses across the Carnegie Mellon University (Pennsylvania) curriculum and beyond, thereby providing an asynchronous,…

  17. A Study of the Committee Structure of Ireland Army Hospital, Fort Knox, Kentucky.

    DTIC Science & Technology

    1980-08-01

    BIBLIOGRAPHY Books Banner, Hubert, Group Dynamics, The Ronald Press Company, N.Y., 1959. Bliss, Edwin C., Getting Things Done, Bantam Books, N.Y., 1978. Carnegie ... Dale , How to Save Time and Get Better Results in Conferences, Dale Carnegie & Associates, Inc., Garden City, N.Y., 1974. Caplow, Theodore, How to

  18. Complexity, Systems, and Software

    DTIC Science & Technology

    2014-08-14

    2014 Carnegie Mellon University Complexity, Systems, and Software Software Engineering Institute Carnegie Mellon University Pittsburgh, PA...this collection of information, including suggestions for reducing this burden, to Washington Headquarters Services , Directorate for Information...OMB control number. 1. REPORT DATE 29 OCT 2014 2. REPORT TYPE N/A 3. DATES COVERED 4. TITLE AND SUBTITLE Complexity, Systems, and Software

  19. Ypsilanti-Carnegie Infant Education Project. Progress Report.

    ERIC Educational Resources Information Center

    Ypsilanti Public Schools, MI.

    Results of the first 6 months of the Ypsilanti-Carnegie Infant Education Project are provided, including quantitative data and a case study, a discussion of the curriculum employed in the home and illustration of curriculum practices, and research design changes. The purpose of the project is to assess the effectiveness of systematic intervention…

  20. Summary of the STIS Cycle 19 Calibration Program

    NASA Astrophysics Data System (ADS)

    Roman-Duval, Julia; Ely, Justin; Aloisi, Alessandra; Oliveira, Cristina; Proffitt, Charles; Hernandez, Svea; Mason, Elena; Sonnetrucker, Paule; Wolfe, Michael; Long, Chris; DiFelice, Audrey; Bostroem, Azalee K.; Holland, Stephen; Lockwood, Sean; Cox, Colin; Wheeler, Thomas

    2014-11-01

    We summarize the Cycle 19 calibration program for the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope, covering the time period November 2011 through October 2012. We give an overview of the whole program, and status summaries for each of the individual proposals comprising the program.

  1. Quasars and the Caltech-Carnegie Connection

    NASA Astrophysics Data System (ADS)

    Waluska, Edward R.

    2007-07-01

    A collaborative relationship existed between the California Institute of Technology (Caltech) and the Carnegie Institution of Washington (Carnegie) beginning in 1946, when a formal agreement was signed between the two groups of trustees. This agreement was designed to integrate Mount Wilson Observatory and the new unfinished Palomar Observatory into a single scientific entity. During the period from 1946 to 1979, much astronomical research was done at both institutions as a direct result of this collaboration. Part of this research included the first identification of a radio source with an apparently stellar object by Allan Sandage of Carnegie and Thomas Matthews of Caltech in 1960, and the first identification of spectral lines at large redshift from a radio source associated with such an object by Maarten Schmidt of Caltech in 1963. This paper examines how the discovery of these objects - which came to be known as quasars - and subsequent research an them, indirectly had an impact an the relationship between Caltech and Carnegie by leading to an environment of increased competitiveness that eventually resulted in the formal dissolution of the relationship in 1980. In this paper, the controversy surrounding the discovery and the interpretation of quasars is examined to provide further understanding about the working relationship when the two institutions were formally collaborating. Some of the data used in this paper were drawn from personal correspondence and interviews with the researchers themselves, and this research forms part of a dissertation for a Ph.D. degree in the Centre for Astronomy at James Cook University, Townsville, Australia.

  2. KSC-02pd0629

    NASA Image and Video Library

    2002-04-30

    KENNEDY SPACE CENTER, FLA. -- At the 2002 Space Congress, Cape Canaveral, Fla., Frank Ceppolina, project manager, Hubble Space Telescope Development Project, gives a presentation on "Hubble Discoveries." The Space Congress is held annually to highlight military and space initiatives, new technologies, and Florida's role in programs and research. This year's theme is Beginning a New Era - Initiatives in Space. NASA presented several paper sessions, including Advancements in Technology. Space Congress is sponsored by the Canaveral Council of Technical Societies

  3. Contributions to the Operating Systems Standards Working Group of the Navy Next Generation Computer Resources Program for FY 1989 - FY 1991

    DTIC Science & Technology

    1991-10-01

    Real - Time Operating System , Hide Tokuda, et al., Carnegie Mellon University "* MARUTI, Hard Real - Time Operating System , Ashok...Architecture, Fred J. Pollack and Kevin C. Kahn, BiiN 10:00 - 10:20 BREAK 10:20 - 12:20 Session VII - Chair: James G. Smith, ONR • A Real - Time Operating System for...Detailed Description * POSIX: Detailed Description * V: Detailed Description * Real - Time Operating System

  4. Flexible Conformable Clamps for a Machining Cell with Applications to Turbine Blade Machining.

    DTIC Science & Technology

    1983-05-01

    PERIOD COVERED * FLEXIBLE CONFORMABLE CLAMPS FOR A MACHINING CELL Interim WITH APPLICATIONS TO TURBINE BLADE MACHINING 6. PERFORMING ORG. REPORT NUMBER...7. AuTmbR(s) 6. CONTRACT OR GRANT NUMBER(a) Eiki Kurokawa 3. PERFORMING ORGANIZATION NAME AND ADDRESS 10. PROGRAM ELE%4NTPROJECT. TASK Carnegie-Mellon...University AREA a WORK UhIT NUMBERS The Robotics Institute Pittsburgh, PA. 15213 II. CONTROLLING OFFICE NAME AND ADDRESS 12. REPORT DATE May 1983. 13

  5. Design and Fabrication of Submicron Magnetic Bubble Device Technology.

    DTIC Science & Technology

    1986-10-31

    interface LPE bubble film GGG substrate Figure 2: Cross section of a silicon on garnet magnetodiode. I : R R R/ B>O0 B 0 z V............. ... ..AV dummy...Carnegie Mellon University, Pittsburgh, Pa 15213. Section I Introduction The main thrust of our LPE garnet film growth program is to develop> films ...shown in Table I and the best choice for an isotropic magnetostrictive film is shown by an asterik. Section IM LPE Film Growth Technique All garnet

  6. NASA Planetary Rover Program

    NASA Technical Reports Server (NTRS)

    Lavery, David; Bedard, Roger J., Jr.

    1991-01-01

    The NASA Planetary Rover Project was initiated in 1989. The emphasis of the work to date has been on development of autonomous navigation technology within the context of a high mobility wheeled vehicle at the JPL and an innovative legged locomotion concept at Carnegie Mellon University. The status and accomplishments of these two efforts are discussed. First, however, background information is given on the three rover types required for the Space Exploration Initiative (SEI) whose objective is a manned mission to Mars.

  7. Exploring the NRO Opportunity for a Hubble-Sized Wide-Field Near-IR Space Telescope - New WFIRST

    NASA Technical Reports Server (NTRS)

    Dressler, Alan; Spergel, David; Mountain, Matt; Postman, Mark; Elliott, Erin; Bendek, Eduardo; Bennett, David; Dalcanton, Julianne; Gaudi, Scott; Gehrels, Neil; hide

    2013-01-01

    We discuss scientific, technical, and programmatic issues related to the use of an NRO 2.4m telescope for the WFIRST initiative of the 2010 Decadal Survey. We show that this implementation of WFIRST, which we call "NEW WFIRST," would achieve the goals of the NWNH Decadal Survey for the WFIRST core programs of Dark Energy and Microlensing Planet Finding, with the crucial benefit of deeper and/or wider near-IR surveys for GO science and a potentially Hubble-like Guest Observer program. NEW WFIRST could also include a coronagraphic imager for direct detection of dust disks and planets around neighboring stars, a high-priority science and technology precursor for future ambitious programs to image Earth-like planets around neighboring stars.

  8. Getting Ideas into Action: Building Networked Improvement Communities in Education. Carnegie Perspectives

    ERIC Educational Resources Information Center

    Bryk, Anthony S.; Gomez, Louis M.; Grunow, Alicia

    2010-01-01

    In this Carnegie essay by Anthony Bryk, Louis Gomez and Alicia Grunow, the authors argue that the social organization of the research enterprise is badly broken and a very different alternative is needed. They instead support a science of improvement research and introduce the idea of a networked improvement community that creates the purposeful…

  9. Carnegie Mellon's STUDIO for Creative Inquiry [and] The Interdisciplinary Teaching Network (ITeN) [and] Interactive Fiction [and] The Networked Virtual Art Museum.

    ERIC Educational Resources Information Center

    Holden, Lynn; And Others

    1992-01-01

    Explains the STUDIO for Creative Inquiry, an interdisciplinary center at Carnegie Mellon University that supports experimental activities in the arts, and its Interdisciplinary Teaching Network. Three STUDIO projects are described: the Ancient Egypt Prototype application of the network; an interactive fiction system based on artificial…

  10. Documenting Community Engagement Practices and Outcomes: Insights from Recipients of the 2010 Carnegie Community Engagement Classification

    ERIC Educational Resources Information Center

    Noel, Jana; Earwicker, David P.

    2015-01-01

    This study was performed to document the strategies and methods used by successful applicants for the 2010 Carnegie Community Engagement Classification and to document the cultural shifts connected with the application process and receipt of the Classification. Four major findings emerged: (1) Applicants benefited from a team approach; (2)…

  11. Higher Inductive Types as Homotopy-Initial Algebras

    DTIC Science & Technology

    2016-08-01

    Higher Inductive Types as Homotopy-Initial Algebras Kristina Sojakova CMU-CS-16-125 August 2016 School of Computer Science Carnegie Mellon University...talk at the Workshop on Logic, Language, Information and Computation (WoLLIC 2011). 1, 2.1 [38] M. Warren. Homotopy-Theoretic Aspects of Constructive Type Theory. PhD thesis, Carnegie Mellon University, 2008. 1 143

  12. Peace through History? The Carnegie Endowment for International Peace's Inquiry into European Schoolbooks, 1921-1924

    ERIC Educational Resources Information Center

    Irish, Tomás

    2016-01-01

    In 1924 the Carnegie Endowment for International Peace published a volume investigating the teaching of school history in former belligerent states in Europe. The project sought to reconcile former enemies through mutual understanding and educational exchange and reflected a widely held belief that although the military conflict had finished, its…

  13. After the Engagement Classification: Using Organization Theory to Maximize Institutional Understandings

    ERIC Educational Resources Information Center

    Thornton, Courtney H.; Zuiches, James J.

    2009-01-01

    Campuses that pursue the Carnegie Community Engagement Classification will in some form take full inventory of their engagement efforts in order to address the range of questions posed by the Carnegie Foundation. At an institution as large, diverse, and decentralized as North Carolina State University, this was no small undertaking. NC State's…

  14. Middle-Level Reform in High- And Low-Performing Middle Schools: A Question of Implementation?

    ERIC Educational Resources Information Center

    Roney, Kathleen; Brown, Kathleen M.; Anfara, Vincent A., Jr.

    2004-01-01

    Although reports calling for middle level schooling reform first appeared in the mid-1970s, change has been slow to come. In Turning Points: Preparing American Youth for the 21st Century (1989), the Carnegie Council on Adolescent Development outlined eight essential elements of middle level education. Drawing from the Carnegie Council's…

  15. An Economic Analysis of Investment in the United States Shipbuilding Industry

    DTIC Science & Technology

    2010-06-01

    using U.S. Bureau of Economic Analysis (BEA) input/output data and the “Leontief inversion process” modeled at Carnegie Mellon University. This... modeled at Carnegie Mellon University. This sector was compared with five alternative investments. Second, the benefits of the shipyard-related...EIO-LCA Model ..................................39 2. Shipyard Direct Labor Trends .........................................................43 viii 3

  16. Parameter Networks: Towards a Theory of Low-level Vision,

    DTIC Science & Technology

    1981-04-01

    8217Iels suc(h ,-s thiose shown in 1ligure 7 to reorganize origami wo.d- figures. Figoure?7. 1’o show an example In detail, Kender’s techn!Ciue for...Compuiter Science Dept, Carnegie-.Mcllon U., October 1979. Kanade, Tl., "A theory of Origami world," CMU-CS-78-144, Computer Science Dept, Carnegie

  17. JPRS Report, East Europe

    DTIC Science & Technology

    1990-04-26

    GERMAN DEMOCRATIC REPUBLIC Legal Provisions on Investment Surveyed [Cologne DEUTSCHLAND ARCHIV Feb] .................. 29 HUNGARY Carnegie Franchise ...131 ZGB), Carnegie Franchise To Be Established in Hungary -weekend cottages, rooms for recreational purposes, 90CHOOO7B Budapest NEPSZABADSAG in...the water breweries. It would be desirable to set up small slaughter- shortage. houses, dairy plants, and bakeries with the participation of foreign

  18. Network Profiling Using Flow

    DTIC Science & Technology

    2012-08-01

    Software Engineering Institute, a federally funded research and development center. Any opinions, findings and conclusions or recommendations...CARNEGIE MELLON UNIVERSITY AND SOFTWARE ENGINEERING INSTITUTE MATERIAL IS FURNISHED ON AN “AS-IS” BASIS. CARNEGIE MELLON UNIVERSITY MAKES NO WARRANTIES OF...required for any other external and/or commercial use. Requests for permission should be directed to the Software Engineering Institute at permission

  19. Best Small Library in America 2009: Union County Carnegie Library, SC--Carolina Dreaming

    ERIC Educational Resources Information Center

    Berry, John N., III

    2009-01-01

    In the past three years, the Union County Carnegie Library (UCCL) in South Carolina has "been transformed." The library board, selected by the county supervisors, knew something had to be done. In October 2005, the board hired Nancy E. Rosenwald as UCCL director. Longing to get back to South Carolina from western Connecticut, Rosenwald…

  20. NASA Astrophysics E/PO: A Quarter Century of Discovery and Inspiration with the Hubble Space Telescope

    NASA Astrophysics Data System (ADS)

    Jirdeh, Hussein; Straughn, Amber; Smith, Denise Anne; Eisenhamer, Bonnie

    2015-08-01

    April 24, 2015 marked the 25th anniversary of the launch of the Hubble Space Telescope. In its quarter-century in orbit, the Hubble Space Telescope has transformed the way we understand the Universe, helped us find our place among the stars, and paved the way to incredible advancements in science and technology.In this presentation, we explain how NASA and ESA, including the Space Telescope Science Institute (STScI) and partners, is using the 25th anniversary of Hubble’s launch as a unique opportunity to communicate to students, educators, and the public the significance of the past quarter-century of discovery with the Hubble Space Telescope. We describe the various programs, resources, and experiences we are utilizing to enhancethe public understanding of Hubble’s many contributions to the scientific world. These include educator professional development opportunities, exhibits, events, traditional and social media, and resources for educators (formal k-12, informal, and higher education). We also highlight how we are capitalizing on Hubble’s cultural popularity to make the scientific connection to NASA’s next Great Observatory, the James Webb Space Telescope.This presentation highlights many of the opportunities by which students, educators, and the public are joining in the anniversary activities, both in-person and online. Find out more at hubble25th.org and follow #Hubble25 on social media.

  1. Obituary: Leonard Searle (1930-2010)

    NASA Astrophysics Data System (ADS)

    Preston, George

    2011-12-01

    Leonard Searle, Astronomer and Director Emeritus of Carnegie Observatories, died at his home on July 2, 2010, in Pasadena, CA, in the midst of a busy retirement that followed a long, distinguished scientific career. Searle was born on October 23, 1930, in the London suburb of Mitcham to parents of modest means. He received his Bachelor of Science degree from University of Saint Andrews in Scotland, and his PhD from Princeton University, where he met his future wife, Eleanor Millard. They were married in Princeton in 1952. Eleanor, his lifelong companion, was a distinguished medieval historian who joined the Division of the Humanities and Social Sciences at Caltech as professor in 1979. She died in 1999. Leonard joined the faculty at University of Toronto in 1953, resigning that position in 1960 to become a Senior Research Fellow at Caltech, where he worked with Jesse Greenstein and Wallace Sargent on the chemical compositions of stars. The Caltech appointment marked the beginning of a fruitful association with Sargent, with whom he published 25 papers. In 1963 Searle left Caltech to join the faculty of the Mount Stromlo Observatory in Australia. Then in 1968 he returned to Pasadena to join the staff of Carnegie Observatories, his final academic home. Several themes punctuate Searle's academic career. One of the most persistent was the abundance of helium in the very early universe, a quantity whose numerical value is of great importance for cosmology. He pursued this topic with Sargent, first in the study of old evolved "horizontal branch" stars. Later, convinced that such stars could not provide a satisfactory answer, he and Sargent turned to certain small galaxies which provided more reliable estimates of the important helium-to-hydrogen abundance ratio. In the pursuit of this answer they devised the "simple model" of chemical evolution, a formalism used by astronomers to this day. He worked with the Dutch astronomer Piet van der Kruit to construct successful models of certain spiral galaxies by careful measurements of surface brightness, and later he worked with colleagues in Pasadena to derive the abundances of chemical elements in primordial stars of our Milky Way Galaxy. His most successful venture was the formulation of a scheme for the assembly of the Milky Way Galaxy from "primordial fragments." This work, which he undertook with then-Carnegie Fellow Robert Zinn, has withstood the test of time. It has been quoted more than 1000 times since it was published in 1978. Searle accepted the Directorship of Carnegie Observatories in 1989 at a signal time in its history. Under his leadership an initial plan to build a single 8.4 meter telescope evolved finally into the construction of two 6.5 meter telescopes, operated since 2000 by a 5-institution consortium at Carnegie's Las Campanas Observatory in Chile. Searle's vital contribution to the Magellan project was his shrewd ability to hire good experts, and then to delegate authority in ways that invited their fruitful participation. All the while, Searle managed to maintain the Observatories' tradition of academic excellence, even as it was plunging into a new world of big-telescope technology. He pursued a visiting scholars program, and he used the important telescope time-allocation process to promote the intellectual growth of Carnegie scientists. His sympathy for the plight of financially strapped Eastern European astronomers took the form of support for the Polish OGLE telescope, to this day a shining success story at Carnegie's Las Campanas Observatory. Following retirement in 1996, Searle continued to follow the progress of the Observatories by frequent contact with his colleagues of many years. He and Eleanor wintered in Pasadena, and during hot Pasadena summers they escaped to their home at Somerset in the south of England. Searle maintained an avid interest in both British and American politics. He has no surviving relatives.

  2. KSC-02pd0626

    NASA Image and Video Library

    2002-04-30

    KENNEDY SPACE CENTER, FLA. -- At the 2002 Space Congress, Cape Canaveral, Fla., attendees listen to a presentation on "Hubble Discoveries" by Frank Ceppolina, project manager, Hubble Space Telescope Development Project. The Space Congress is held annually to highlight military and space initiatives, new technologies, and Florida's role in programs and research. This year's theme is Beginning a New Era - Initiatives in Space. NASA presented several paper sessions, including Advancements in Technology. Space Congress is sponsored by the Canaveral Council of Technical Societies

  3. Correlation of the Hubble Space Telescope (HST) Space Telescope Imaging Spectrometer (STIS) On-Orbit Data with Pre-launch Predictions and Ground Contamination Controls

    NASA Technical Reports Server (NTRS)

    Hansen, Patricia A.

    2003-01-01

    The Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) was deployed on-orbit in February 1997. The contamination program for STIS was stringently controlled as the five-year end-of-life deposition was set at 158, per optical element. Contamination was controlled through materials selection, extensive vacuum outgassing certifications, cleaning techniques, and environmental controls. In addition to ground contamination controls, on-orbit contamination controls were implemented for both the HST servicing mission activities and early post-servicing mission checkout. The extensive contamination control program will be discussed and the STIS on-orbit data will be correlated with the prelaunch analytical predictions.

  4. Human Space Flight Plans Committee

    NASA Image and Video Library

    2009-06-16

    Norman Augustine, chair of the Human Space Flight Review Committee, listens to a comment from the audience during the first of several public meetings at different U.S. locations, Wednesday, June 17, 2009, at the Carnegie Institution in Washington. The panel will examine ongoing and planned NASA development activities and potential alternatives in order to present options for advancing a safe, innovative, affordable and sustainable human space flight program following the space shuttle's retirement. The committee wil present its results by August 2009. Photo Credit: (NASA/Paul E. Alers)

  5. Human Space Flight Plans Committee

    NASA Image and Video Library

    2009-06-16

    Norman Augustine, chair of the Human Space Flight Review Committee, makes a point during the first of several public meetings at different U.S. locations, Wednesday, June 17, 2009, at the Carnegie Institution in Washington. The panel will examine ongoing and planned NASA development activities and potential alternatives in order to present options for advancing a safe, innovative, affordable and sustainable human space flight program following the space shuttle's retirement. The committee wil present its results by August 2009. Photo Credit: (NASA/Paul E. Alers)

  6. The AEMS (Analysis of Electrical and Mechanical Systems) Project in Applied Mathematics at Carnegie-Mellon University.

    DTIC Science & Technology

    1982-12-01

    Nishizeki 0. Wyler J. M. Greenberg W. Noll Z. Zener H. J. Greenberg J. J. Oravec 5 IV. History of the AENIS Project (1950-1960) Prior to the second...of Professor Herbert Greenberg they drafted a proposal for a research project. The goal of this project was not only to solve certain research...active program in wave research was continued by Professors MacCamy, Mizel, and Greenberg . Their work has directly related to the AEMS work in the

  7. A Conversation with Lee Shulman--Signature Pedagogies for Teacher Education: Defining Our Practices and Rethinking Our Preparation

    ERIC Educational Resources Information Center

    Falk, Beverly

    2006-01-01

    Lee S. Shulman is the President of The Carnegie Foundation for the Advancement of Teaching, a foundation whose mission is "to do and perform all things necessary to encourage, uphold and dignify the profession of teaching." Prior to assuming his role at Carnegie, Shulman was the Charles E. Ducommun Professor of Education at Stanford…

  8. Annual Report of the Carnegie Corporation of New York 1972.

    ERIC Educational Resources Information Center

    Carnegie Corp. of New York, NY.

    This annual report of the Carnegie Corporation presents a listing of the grants made by the corporation during the fiscal year ended September 1972; a listing of books published as a result of the grants awarded during that year; the general report of the secretary for the year; and the report of the treasurer including the accountants' opinion of…

  9. Clergy of the Mind: Alvin S. Johnson, William S. Learned, the Carnegie Corporations, and the American Library Association

    ERIC Educational Resources Information Center

    Latham, Joyce M.

    2010-01-01

    During the early twentieth century, Alvin Johnson and William S. Learned produced two separate but related studies relative to the donations of the Carnegie Corporation of New York (CCNY) to public library construction. These reports became means for the planned disassociation of the philanthropic organization from its historical relationship with…

  10. Science, Technology, Engineering and Math (STEM) Academic Librarian Positions during 2013: What Carnegie Classifications Reveal about Desired STEM Skills

    ERIC Educational Resources Information Center

    Trei, Kelli

    2015-01-01

    This study analyzes the requirements and preferences of 171 science, technology, engineering, and math (STEM) academic librarian positions in the United States as advertised in 2013. This analysis compares the STEM background experience preferences with the Carnegie rankings of the employing institution. The research examines the extent to which…

  11. ABCs of Operational Resilience

    DTIC Science & Technology

    2014-01-23

    Mission Success To be operationally resilient, cyber- and/or kinetic-enabled missions must address operational risk on a number of “planes...man ement, protection, and s stainme t begin. CERT® Operational Resilience: Manage, Protect, and Sustain Twitter #CERTopRES © 2014 Carnegie... t c e t ee Lo e CERT I Software Engineering Institute I CarnegieMellonUniversity CERT® Operational Resilience: Manage, Protect, and Sustain

  12. Opportunity by Design: New High School Models for Student Success. Carnegie Challenge

    ERIC Educational Resources Information Center

    Hamilton, Leah; Mackinnon, Anne

    2013-01-01

    The goal of Carnegie "Challenge" papers is to lift up ideas and issues in a way that elevates them to the nation's agenda. This paper is a "Challenge" paper, and serves as a call to realize the full power of the Common Core by redesigning and reshaping schools to support teachers and maximize key resources, rather than…

  13. A Digest of Reports of the Carnegie Commission on Higher Education. With an Index to Recommendations and Suggested Assignments of Responsibility for Action.

    ERIC Educational Resources Information Center

    Carnegie Commission on Higher Education , Berkeley, CA.

    In 21 reports issued over the span of almost six years, the Carnegie Commission on Higher Education has made available a massive resource of information for policymakers in colleges and universities, government agencies, and philanthropic and business organizations. The Commission has also offered nearly 300 individual recommendations for…

  14. To Dignify the Profession of the Teacher: The Carnegie Foundation Celebrates 100 Years

    ERIC Educational Resources Information Center

    Shulman, Lee S.

    2005-01-01

    Serious work on education is never just a work of the moment. Some problems are the consequences of yesterday's solutions, and many of the most promising approaches to today's issues build on the efforts of earlier generations. In short, the work that is going on presently at The Carnegie Foundation for the Advancement of Teaching must be…

  15. Starting Where the People Are: The African Medical and Research Foundation (AMREF). Carnegie Quarterly, Volume XXXII, Number 2.

    ERIC Educational Resources Information Center

    Carnegie Quarterly, 1987

    1987-01-01

    This issue of the "Carnegie Quarterly" describes three projects that are being conducted by the African Medical and Research Foundation (AMREF). The projects are the following: (1) building community participation in health care at Lake Kenyatta; (2) the role of community education in disease control among the Turkana people at…

  16. Devils in Disguise: The Carnegie Project, the Cherokee Nation, and the 1960s

    ERIC Educational Resources Information Center

    Cobb, Daniel M.

    2007-01-01

    In this article, the author talks about the experiences of many of the people involved in the Carnegie Project, an effort in the 1960s to establish ties with the "tribal community"--people who spoke Cherokee as their first language and lived in small kin-related settlements spread across five counties in northeastern Oklahoma--and…

  17. Collaborative Autonomy with Group Autonomy for Mobile Systems (GAMS)

    DTIC Science & Technology

    2014-11-18

    Carnegie Mellon University for the operation of the Software Engineering Institute, a federally funded research and development center. Any opinions...tutorials, doxygen) Intro MADARA GAMS Conclusion 9 James Edmondson © 2014 Carnegie Mellon University How MADARA helps researchers and developers...architecture portability to prevent vendor lock-in and shorten transition timeframe • Open source. Free. Extensible. • Allows reseachers to focus

  18. Summary of the COS Cycle 20 Calibration Program

    NASA Astrophysics Data System (ADS)

    Roman-Duval, Julia; Aloisi, Alessandra; Bostroem, K. Azalee; Ely, Justin; Holland, Stephen; Lockwood, Sean; Oliveira, Cristina; Penton, Steven; Proffitt, Charles; Sahnow, David; Sonnentrucker, Paule; Welty, Alan D.; Wheeler, Thomas

    2015-06-01

    We summarize the Cycle 20 calibration program for the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope, covering the time period from November 2012 through October 2013. We give an overview of the Calibration plan and status summaries for each of the individual proposals comprising the C20 Calibration program.

  19. Summary of the COS Cycle 21 Calibration Program

    NASA Astrophysics Data System (ADS)

    Sana, Hugues; Fox, Andrew; Roman-Duval, Julia; Ely, Justin; Bostroem, K. Azalee; Lockwood, Sean; Oliveira, Cristina; Penton, Steve; Proffitt, Charles; Sahnow, David; Sonnentrucker, Paule; Welty, Alan D.; Wheeler, Thomas

    2015-09-01

    We summarize the Cycle 21 calibration program for the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope, covering the time period from November 2013 through October 2014. We give an overview of the Calibration plan and status summaries for each of the individual proposals comprising the C21 Calibration program.

  20. Local gravitational physics of the Hubble expansion. Einstein's equivalence principle in cosmology

    NASA Astrophysics Data System (ADS)

    Kopeikin, Sergei M.

    2015-01-01

    We study physical consequences of the Hubble expansion of Friedmann-Lemaıtre-Robertson-Walker (FLRW) manifold on measurement of space, time and light propagation in the local inertial frame. We use the results of this study to analyse the Solar System radar ranging and Doppler tracking experiments and time synchronization. FLRW manifold is covered by the coordinates ( t, y i ), where t is the cosmic time coinciding with the proper time of the Hubble observers and identified with the barycentric coordinate time (TCB) used in ephemeris astronomy. We introduce the local inertial coordinates x α = ( x 0, x i ) in the vicinity of a world line of a Hubble observer with the help of a special conformal transformation that respects the local equivalence between the tangent and FLRW manifold. The local inertial metric is Minkowski flat and is materialized by the congruence of time-like geodesics of static observers being at rest with respect to the local spatial coordinates x i . The static observers are equipped with the ideal clocks measuring their own proper time which is synchronized with the cosmic time t measured by the Hubble observer. We consider the geodesic motion of test particles and notice that the local coordinate time x 0 = x 0( t) taken as a parameter along the world line of the particle, is a function of Hubble's observer time t. This function changes smoothly from x 0 = t for a particle at rest (observer's clock), to x 0 = t + (1/2) Ht 2 for photons, where H is the Hubble constant. Thus, the motion of a test particle is non-uniform when its world line is parametrized by the cosmic time t. NASA JPL Orbit Determination Program operates under the assumption that the spacetime is asymptotically flat which presumes that the motion of light (after the Shapiro delay is excluded) is uniform with respect to the time t but it does not comply with the non-uniform motion of light on cosmological manifold. For this reason, the motion of light in the Solar System analysed with the Orbit Determination Program appears as having a systematic blue shift of frequency, of radio waves circulating in the Earth-spacecraft radio link. The magnitude of the anomalous blue shift of frequency is proportional to the Hubble constant H that may open an access to the measurement of this fundamental cosmological parameter in the Solar System radiowave experiments.

  1. NASA Astrophysics Education and Public Outreach: The Impact of the Space Telescope Science Institute Office of Public Outreach

    NASA Astrophysics Data System (ADS)

    Smith, Denise Anne; Jirdeh, Hussein; Eisenhamer, Bonnie; Villard, Ray; Green, Joel David

    2015-08-01

    As the science operations center for the Hubble Space Telescope and the James Webb Space Telescope, the Space Telescope Science Institute (STScI) is uniquely positioned to captivate the imagination and inspire learners of all ages in humanity’s quest to understand fundamental questions about our universe and our place in it. This presentation will provide an overview of the impact of the STScI’s Office of Public Outreach’s efforts to engage students, educators, and the public in exploring the universe through audience-based news, education, and outreach programs.At the heart of our programs lies a tight coupling of scientific, education, and communications expertise. By partnering scientists and educators, we assure current, accurate science content and education products and programs that are classroom-ready and held to the highest pedagogical standards. Likewise, news and outreach programs accurately convey cutting-edge science and technology in a way that is attuned to audience needs. The combination of Hubble’s scientific capabilities, majestic imagery, and our deep commitment to create effective programs to share Hubble science with the education community and the public, has enabled the STScI Office of Public Outreach programs to engage 6 million students and ½ million educators per year, and 24 million online viewers per year. Hubble press releases generate approximately 5,000 online news articles per year with an average circulation of 125 million potential readers per press release news story. We will also share how best practices and lessons learned from this long-lived program are already being applied to engage a new generation of explorers in the science and technology of the James Webb Space Telescope.

  2. Hubble Captures Vivid Auroras in Jupiter’s Atmosphere

    NASA Image and Video Library

    2017-12-08

    Astronomers are using the NASA/ESA Hubble Space Telescope to study auroras — stunning light shows in a planet’s atmosphere — on the poles of the largest planet in the solar system, Jupiter. This observation program is supported by measurements made by NASA’s Juno spacecraft, currently on its way to Jupiter. Jupiter, the largest planet in the solar system, is best known for its colorful storms, the most famous being the Great Red Spot. Now astronomers have focused on another beautiful feature of the planet, using Hubble's ultraviolet capabilities. The extraordinary vivid glows shown in the new observations are known as auroras. They are created when high-energy particles enter a planet’s atmosphere near its magnetic poles and collide with atoms of gas. As well as producing beautiful images, this program aims to determine how various components of Jupiter’s auroras respond to different conditions in the solar wind, a stream of charged particles ejected from the sun. This observation program is perfectly timed as NASA’s Juno spacecraft is currently in the solar wind near Jupiter and will enter the orbit of the planet in early July 2016. While Hubble is observing and measuring the auroras on Jupiter, Juno is measuring the properties of the solar wind itself; a perfect collaboration between a telescope and a space probe. “These auroras are very dramatic and among the most active I have ever seen”, said Jonathan Nichols from the University of Leicester, U.K., and principal investigator of the study. “It almost seems as if Jupiter is throwing a firework party for the imminent arrival of Juno.” Read more: go.nasa.gov/294QswK Credits: NASA, ESA, and J. Nichols (University of Leicester)

  3. Hubble Captures Vivid Auroras in Jupiter’s Atmosphere

    NASA Image and Video Library

    2016-06-30

    Astronomers are using the NASA/ESA Hubble Space Telescope to study auroras — stunning light shows in a planet’s atmosphere — on the poles of the largest planet in the solar system, Jupiter. This observation program is supported by measurements made by NASA’s Juno spacecraft, currently on its way to Jupiter. Jupiter, the largest planet in the solar system, is best known for its colorful storms, the most famous being the Great Red Spot. Now astronomers have focused on another beautiful feature of the planet, using Hubble's ultraviolet capabilities. The extraordinary vivid glows shown in the new observations are known as auroras. They are created when high-energy particles enter a planet’s atmosphere near its magnetic poles and collide with atoms of gas. As well as producing beautiful images, this program aims to determine how various components of Jupiter’s auroras respond to different conditions in the solar wind, a stream of charged particles ejected from the sun. This observation program is perfectly timed as NASA’s Juno spacecraft is currently in the solar wind near Jupiter and will enter the orbit of the planet in early July 2016. While Hubble is observing and measuring the auroras on Jupiter, Juno is measuring the properties of the solar wind itself; a perfect collaboration between a telescope and a space probe. “These auroras are very dramatic and among the most active I have ever seen”, said Jonathan Nichols from the University of Leicester, U.K., and principal investigator of the study. “It almost seems as if Jupiter is throwing a firework party for the imminent arrival of Juno.” Credits: NASA, ESA, and J. Nichols (University of Leicester)

  4. Hubble Observations of the Exomoon Candidate Kepler-1625b I

    NASA Astrophysics Data System (ADS)

    Teachey, Alexander; Kipping, David; Torres, Guillermo; Bakos, Gaspar A.; Nesvorný, David; Buchhave, Lars; Huang, Chelsea Xu; Hartman, Joel D.

    2018-01-01

    The exomoon candidate Kepler-1625b I was identified by the Hunt for Exomoons with Kepler (HEK) collaboration in August 2016 following an extensive program to characterize the occurrence rate of exomoons. Follow-up observations of the candidate for the purpose of validating the existence of the moon and constraining its properties were carried out on the Hubble Space Telescope on October 28th-29th 2017, using slitless spectroscopy on Wide Field Camera 3. We report preliminary results of that observation.

  5. The Hubble Space Telescope Servicing Mission 3A Contamination Control Program

    NASA Technical Reports Server (NTRS)

    Hansen, Patricia A.

    2000-01-01

    After nearly 10 years on-orbit, the Hubble Space Telescope (HST) external thermal control materials and paint have degraded due to exposure to the low Earth orbit environment. This presented a potentially large on-orbit contamination source (particles and/or debris). Contamination mitigation techniques were developed to augment existing on-orbit servicing contamination controls. They encompassed mission management, crew training, and crew aids and tools. These techniques were successfully employed during the HST Servicing Mission 3A, December 1999.

  6. Finding Our Origins with the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2003-01-01

    NASA's Origins program is a series of space telescopes designed to study the origins of galaxies, stars, planets and life in the universe. In this talk, I will concentrate on the origin and evolution of galaxies, beginning with the Big Bang and tracing what we have learned with the Hubble Space Telescope through to the present day. I will introduce several of the tools that astronomers use to measure distances, measure velocities, and look backwards in time. I will show that results from studies with Hubble have led to plans for its successor, the James Webb Space Telescope, which is designed to find the first galaxies that formed in the distant past. I will finish with a short discussion of other missions in the Origins theme, including the Terrestrial Planet Finder.

  7. Finding our Origins with the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2004-01-01

    NASA s Origins program is a series of space telescopes designed to study the origins of galaxies, stars, planets and life in the universe. In this talk, I will concentrate on the origin and evolution of galaxies, beginning with the Big Bang and tracing what we have learned with the Hubble Space Telescope through to the present day. I will introduce several of the tools that astronomers use to measure distances, measure velocities, and look backwards in time. I will show that results from studies with Hubble have led to plans for its successor, the James Webb Space Telescope, which is designed to find the first galaxies that formed in the distant past. I will finish with a short discussion of other missions in the Origins theme, including the Terrestrial Planet Finder.

  8. The Ambivalence of the Israeli Academic Profession: Research vs. Teaching. The Academic Profession Approaches the Twenty-First Century: the Carnegie Foundation International Survey, Symposium.

    ERIC Educational Resources Information Center

    Gottlieb, Esther E.; And Others

    Attitudes of Israeli senior faculty concerning research and teaching were evaluated using the Carnegie international questionnaire. Approximately one third of the total faculty population in Israel was randomly sampled, but stratified by institutional size. The questionnaire was sent to 2,225 faculty and 502 returned completed forms (22.56…

  9. Question Generation via Overgenerating Transformations and Ranking

    DTIC Science & Technology

    2009-01-01

    School of Computer Science Carnegie Mellon University 5000 Forbes Ave., Pittsburgh, PA 15213 www.lti.cs.cmu.edu c©2009, Michael Heilman and Noah A...PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) Carnegie Mellon University ,School of Computer Science,5000 Forbes Ave,Pittsburgh,PA,15213 8...1967), in particular those that view a question as a transformation of a canonical declarative sentence ( Chomsky , 1973). In computational linguistics

  10. Private Power for the Public Good. A History of the Carnegie Foundation for the Advancement of Teaching. [Revised.

    ERIC Educational Resources Information Center

    Lagemann, Ellen Condliffe

    This book traces the history of the Carnegie Foundation for the Advancement of Teaching from its founding in 1906 through 1979. A 1999 foreword by the current president of the Foundation notes the influence of the book and briefly updates the foundation's history. The foreword reiterates the book's judgment that the foundation's policies typically…

  11. Holt Social Studies Curriculum. Developed by Carnegie Social Studies Curriculum Development Center, Carnegie-Mellon University. Product Development Report 13.

    ERIC Educational Resources Information Center

    Sanderson, Barbara A.; Kratochvil, Daniel W.

    This report is the thirteenth of twenty-one reports dealing with the developmental history of a recent educational product: the Holt Social Studies Curriculum directed by Dr. Edwin Fenton. This series of courses stresses an inquiry approach to the study of history and the social sciences, specifically economic and political systems, world history,…

  12. Theory and Applications of Computational Time-Reversal Imaging

    DTIC Science & Technology

    2007-05-03

    experimental data collected by a research team from Carnegie Mellon University illustrating the use of the algorithms developed in the project. The final...2.1 Early Results from CMU experimental data ..... ................... 4 2.1.1 Basic Time Reversal Imaging ....... ...................... 4 2.1.2 Time... experimental data collected by Carnegie Mellon University illustrating the use of the algorithms developed in the project. 15. SUBJECT TERMS 16. SECURITY

  13. A Foundation's Story: The First Seventy-Five Years of the Carnegie Foundation for the Advancement of Teaching.

    ERIC Educational Resources Information Center

    Piefer, Alan

    The history of The Carnegie Foundation for the Advancement of Teaching (CFAT) is traced. Three eras are described: 1905 to 1930, a period of initial creativity and influence; 1930 to 1966, a period of gradual decline, leading eventually to loss of independence and virtual extinction; and 1966 to 1979, a period of revitalization. Originally, CFAT…

  14. Synopsis of the Carnegie Report on Teaching: "A Nation Prepared: Teachers for the 21st Century."

    ERIC Educational Resources Information Center

    Lake, Sara

    This review of the Carnegie Report on Teaching, "A Nation Prepared: Teachers for the 21st Century" presents an overview the report's goals for the future of the teaching profession. Written by the Task Force on Teaching as a Profession, the report goal's were to: (1) remind America of its economic challenges; (2) "assert the primacy…

  15. The Far-Field Hubble Constant

    NASA Astrophysics Data System (ADS)

    Lauer, Tod

    1995-07-01

    We request deep, near-IR (F814W) WFPC2 images of five nearby Brightest Cluster Galaxies (BCG) to calibrate the BCG Hubble diagram by the Surface Brightness Fluctuation (SBF) method. Lauer & Postman (1992) show that the BCG Hubble diagram measured out to 15,000 km s^-1 is highly linear. Calibration of the Hubble diagram zeropoint by SBF will thus yield an accurate far-field measure of H_0 based on the entire volume within 15,000 km s^-1, thus circumventing any strong biases caused by local peculiar velocity fields. This method of reaching the far field is contrasted with those using distance ratios between Virgo and Coma, or any other limited sample of clusters. HST is required as the ground-based SBF method is limited to <3,000 km s^-1. The high spatial resolution of HST allows precise measurement of the SBF signal at large distances, and allows easy recognition of globular clusters, background galaxies, and dust clouds in the BCG images that must be removed prior to SBF detection. The proposing team developed the SBF method, the first BCG Hubble diagram based on a full-sky, volume-limited BCG sample, played major roles in the calibration of WFPC and WFPC2, and are conducting observations of local galaxies that will validate the SBF zeropoint (through GTO programs). This work uses the SBF method to tie both the Cepheid and Local Group giant-branch distances generated by HST to the large scale Hubble flow, which is most accurately traced by BCGs.

  16. Completing the Legacy of Hubble's Wide/Deep Fields: An Aligned Complete Dataset of 1220 Orbits on the GOODS-N/CANDELS-N Region

    NASA Astrophysics Data System (ADS)

    Illingworth, Garth

    2017-08-01

    The GOODS-N/CANDELS-N region is second only to the GOODS-S/ECDF-S region in the extent of its HST and Spitzer coverage, making it a remarkable science resource. Yet of 1220 orbits of ACS and WFC3/IR imaging from 27 programs on the GOODS-N region, fully 42% of the total, about 520 orbits of imaging data from 22 programs, remains unavailable in MAST as a high-level science data product (HLSP). The GOODS-N region dataset is a key Legacy field ( 3 Msec from HST, 6 Msec from Spitzer, and 2 Msec from Chandra). We propose to deliver, with catalogs, HST ACS and WFC3/IR HLSPs to MAST for all 1220 orbits of GOODS-N data. We will also deliver HLSPs for the EGS, UDS and the COSMOS CANDELS regions, including new data not included to date. These four HLSPs, 2300 orbits of HST data ( 75% of a HST Cycle ), will add substantially to (1) our understanding of the build-up of galaxies to z 6 in the first Gyr during reionization, (2) the development of galaxies over the subsequent Gyr to the peak of the star formation rate in the universe at z 2-3, and (3) the transition at z<2 of early star-forming galaxies to the full splendor of the Hubble sequence. We can do this major AR Legacy program, having submitted a HLSP of ALL 2442 orbits of HST data on the GOODS- S region (>950 orbits new). The total volume of data in the GOODS-S Hubble Legacy Field (HLF-GOODS-S) is 5.8 Msec in 7211 exposures ( 70% of a HST cycle). The HLF-GOODS-S includes 4 new deep areas akin to the HUDF/XDF. The four proposed NEW Hubble Legacy Field datasets will complement the Frontier Field datasets and our recent HLF-GOODS-S and HUDF/XDF HLSP submissions. They will be cornerstones of Hubble's Legacy as the JWST era dawns.

  17. The Carnegie Dietary Survey of Interwar Britain.

    PubMed

    Shave, Samantha A

    2015-01-01

    This research note describes an under-used collection of papers which document interwar income, nutrition and health in Britain which were created in the administration of the Carnegie Dietary Survey by John Boyd-Orr in the Rowett Institute with funding from the Carnegie United Kingdom Trust. The survey was conducted in 16 rural and urban places across England and Scotland between 1937-9, and are now held at the Specialist Collections Centre at the University of Aberdeen. While the importance of the survey in informing knowledge about nutrition and the development of rationing has been acknowledged in the field of social medicine, the survey data has primarily been used by epidemiological scientists and economic historians. After outlining the survey's past influences and uses, this item details the possible ways the data could be used by social, economic and local population historians.

  18. Data Integration: Charting a Path Forward to 2035

    DTIC Science & Technology

    2011-02-14

    New York, NY: Gotham Books, 2004. Seligman , Len. Mitre Corporation, e-mail interview, 6 Dec 2010. Singer, P.W. Wired for War: The Robotics...articles.aspx (accessed 4 Dec 2010). Ultra-Large-Scale Systems: The Software Challenge of the Future. Study lead Linda Northrup. Pittsburgh, PA: Carnegie...Virtualization?‖ 1. 41 Ultra-Large-Scale Systems: The Software Challenge of the Future. Study lead Linda Northrup. Pittsburgh, PA: Carnegie Mellon Software

  19. Using TSP to Improve Performance

    DTIC Science & Technology

    2008-11-13

    Carnegie Mellon University Using TSP to Improve Performance 46 Work - Life Balance People are your most important resource. Finding and retaining good people...is critical to long-term success. Intuit found that TSP improved work - life balance , a key factor in job satisfaction. Source: Intuit © 2008 Carnegie...Mellon University Using TSP to Improve Performance 47 Intuit TSP Survey Results Improved work - life balance with TSP is reflected in job satisfaction

  20. Exploring the Relationship between Patron Type, Carnegie Classification, and Satisfaction with Library Services: An Analysis of LibQUAL+® Results

    ERIC Educational Resources Information Center

    Guder, Christopher S.

    2012-01-01

    The purpose of this study was to explore how faculty and students responded to the Information Control section of the LibQUAL+® survey at two libraries with different Carnegie Classifications. As one of the institutions being studied was considering a shift from a research institution to one more focused on teaching and learning, this study used…

  1. I Love My Librarian Award: An Award That Recognizes Great Librarians Also Highlights the Central Role of Libraries in Communities across America. Carnegie Results

    ERIC Educational Resources Information Center

    Deutsch, Abigail

    2013-01-01

    The Carnegie Corporation of New York/"New York Times" I Love My Librar­ian Award publicizes librarians' abilities to improve their communities, and by highlighting the achievements of the winners, inspire other librarians to boost their own performance. Since the award's creation in 2008, it has helped the public to better understand…

  2. Wireless Emergency Alerts Commercial Mobile Service Provider (CMSP) Cybersecurity Guidelines

    DTIC Science & Technology

    2016-06-16

    Distribution Statement A: Approved for Public Release; Distribution is Unlimited Copyright 2016 Carnegie Mellon University This material is based upon...opinions, findings and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views...INSTITUTE MATERIAL IS FURNISHED ON AN “AS-IS” BASIS. CARNEGIE MELLON UNIVERSITY MAKES NO WARRANTIES OF ANY KIND, EITHER EXPRESSED OR IMPLIED, AS TO

  3. Home Computer and Internet User Security

    DTIC Science & Technology

    2005-01-01

    Information Security Model © 2005 Carnegie Mellon University (Lawrence R. Rogers, Author) Home Computer and Internet User Security...Carnegie Mellon University (Lawrence R. Rogers, Author) Home Computer and Internet User Security Version 1.0.4 – slide 50 Contact Information Lawrence R. Rogers • Email: cert@cert.org CERT website: http://www.cert.org/ ...U.S. Patent and Trademark Office Home Computer and Internet User Security Report Documentation Page Form ApprovedOMB

  4. Toward a Global Community of Scholars. The Special Partnership between the Carnegie Foundation for the Advancement of Teaching and China's National Center for Education Development Research, 1988-1997.

    ERIC Educational Resources Information Center

    Ch'i, Hsi-sheng

    This volume traces the history of a collaboration between the Carnegie Foundation for the Advancement of Teaching and China's National Center for Education Development Research. The collaboration, which began in 1988, was initiated to conduct a comparative study of education in the two countries through information exchanges and seminars.…

  5. Acquisition Review Quarterly (ARQ), Volume 1 Number 3, Summer 1994

    DTIC Science & Technology

    1994-01-01

    sole- and dual-source production and their cost implications , and suggests the use of explicit demand curves. 281 - GUIDELINES FOR AUTHORS...millions of square miles of the American landscape. If you look at a map, it is astonishing how much of the country we cover. Naturally, nearly every- thing...See Carnegie Commission Report, Facing Towards Governments - Nongovernmental Organi- zations and Scientific and Technical Advice (New York: Carnegie

  6. Opponent Modeling in Interesting Adversarial Environments

    DTIC Science & Technology

    2008-07-01

    University of Alberta and the research team at Carnegie Melon University have both explored various abstraction and solution techniques. In [10] Billings et...solution for an abstraction of the entire four-betting-round version of Limit Texas Hold’em. At Carnegie Melon University, Gilpin and Sandholm...measuring how well opponent models met these goals. We’ve found that modeling opponents that adapt while playing is an active and fertile field of

  7. A Survey of Commonly Applied Methods for Software Process Improvement

    DTIC Science & Technology

    1994-02-01

    conducted a controlled experimental study of the effectiveness of the method. They compared 10 cleanroom teams with 5 non -cleanroom teams working for six...Robert D. Austin Doctoral Candidate Carnegie Mellon University Daniel J. Paulish Resident Affiliate Siemens Corporate Research , Inc. Accesion For0...the U.S. Department of Defense. Copyright 0 1994 by Carnegie Mellon University. Copies of the documen are available from Research Access. Iinc., 800

  8. Taking Advantage of Agile while Minimizing Risk: User Stories and Other Fables

    DTIC Science & Technology

    2013-11-20

    and inability to deliver 24 © 2013 Carnegie Mellon University Scrum practices are said to depend on each other and should not be changed We...identified two mismatches between Scrum and the studied organization Mismatches we identified were considered necessary or even beneficial Changes to... Scrum cannot categorically be considered detrimental ScrumButs What about modifying SCRUM ? 25 © 2013 Carnegie Mellon University Microsoft Research

  9. Information Security Is a Business Continuity Issue: Are You Ready

    DTIC Science & Technology

    2015-05-09

    and data files • Legal - Employees have filed four lawsuits against the company for not protecting their data • Breach Expenses - In its first quarter...incidents into their planning, testing, and execution processes. 28© 2015 Carnegie Mellon University Factors Affecting Cost of Data Breach SOURCE: Ponemon...2014 Cost of Data Breach Study Per Capita Cost 29© 2015 Carnegie Mellon University Thank you for your attention.

  10. Calls for reform of medical education by the Carnegie Foundation for the Advancement of Teaching: 1910 and 2010.

    PubMed

    Irby, David M; Cooke, Molly; O'Brien, Bridget C

    2010-02-01

    The Carnegie Foundation for the Advancement of Teaching, which in 1910 helped stimulate the transformation of North American medical education with the publication of the Flexner Report, has a venerated place in the history of American medical education. Within a decade following Flexner's report, a strong scientifically oriented and rigorous form of medical education became well established; its structures and processes have changed relatively little since. However, the forces of change are again challenging medical education, and new calls for reform are emerging. In 2010, the Carnegie Foundation will issue another report, Educating Physicians: A Call for Reform of Medical School and Residency, that calls for (1) standardizing learning outcomes and individualizing the learning process, (2) promoting multiple forms of integration, (3) incorporating habits of inquiry and improvement, and (4) focusing on the progressive formation of the physician's professional identity. The authors, who wrote the 2010 Carnegie report, trace the seeds of these themes in Flexner's work and describe their own conceptions of them, addressing the prior and current challenges to medical education as well as recommendations for achieving excellence. The authors hope that the new report will generate the same excitement about educational innovation and reform of undergraduate and graduate medical education as the Flexner Report did a century ago.

  11. Application of Carnegie stages of development to unify human and baboon ultrasound findings early in pregnancy.

    PubMed

    Santolaya-Forgas, Joaquin; De Leon-Luis, Juan; Friel, Lara A; Wolf, Roman

    2007-09-01

    The objective of this study was to determine if very early ultrasonographic measurements obtained from human and baboon are comparable. For this purpose, the gestational, amniotic and yolk sacs, embryonic crown rump length (CRL) and heart rate were measured ultrasonographically between 35 and 47 days from the mean day of a three-day mating period in baboons (n=18) and between 42 to 58 days from fertilization as calculated from the CRL measurements in human pregnancies (n=82). Ultrasonographic measurements from both species were then plotted in the same graph using Carnegie stages of embryonic development as the independent variable to allow for visual comparisons. Mean gestational age at ultrasonographic studies was significantly different for humans and baboons (50.4 vs. 41 days, respectively; p>0.01). Significant correlations (p>0.01) were noted between ultrasonographic measurements and Carnegie stages of development in both humans and baboons. Only the gestational and the yolk sacs were significantly smaller in baboons than in humans (p>0.05). The findings that embryonic CRL, extra-embryonic space and heart rate are very similar between the 17th and 23rd Carnegie developmental stages make the baboon a promising surrogate of human pregnancy for investigations using celocentesis.

  12. Program maintenance manual for nickel cadmium battery expert system, version 1

    NASA Technical Reports Server (NTRS)

    1986-01-01

    The Nickel-Cadmium Battery Expert System (NICBES) is an expert system for fault diagnosis and advice of the nickel-cadmium batteries found in the Hubble Space Telescope (HST). The system application and security, equipment environment, and the program maintenance procedures are examined.

  13. Hubble Space Telescope Program on STS-95 Supported by Space Acceleration Measurement System for Free Flyers

    NASA Technical Reports Server (NTRS)

    Kacpura, Thomas J.

    2000-01-01

    John Glenn's historic return to space was a primary focus of the STS 95 space shuttle mission; however, the 83 science payloads aboard were the focus of the flight activities. One of the payloads, the Hubble Space Telescope Orbital System Test (HOST), was flown in the cargo bay by the NASA Goddard Space Flight Center. It served as a space flight test of upgrade components for the telescope before they are installed in the shuttle for the next Hubble Space Telescope servicing mission. One of the upgrade components is a cryogenic cooling system for the Near Infrared Camera and Multi-Object Spectrometer (NICMOS). The cooling is required for low noise in the receiver's sensitive electronic instrumentation. Originally, a passive system using dry ice cooled NICMOS, but the ice leaked away and must be replaced. The active cryogenic cooler can provide the cold temperatures required for the NICMOS, but there was a concern that it would create vibrations that would affect the fine pointing accuracy of the Hubble platform.

  14. Results of a technical analysis of the Hubble Space Telescope nickel-cadmium and nickel-hydrogen batteries

    NASA Technical Reports Server (NTRS)

    Manzo, Michelle A.

    1991-01-01

    The Hubble Space Telescope (HST) Program Office requested the expertise of the NASA Aerospace Flight Battery Systems Steering Committee (NAFBSSC) in the conduct of an independent assessment of the HST's battery system to assist in their decision of whether to fly nickel-cadmium or nickel-hydrogen batteries on the telescope. In response, a subcommittee to the NAFBSSC was organized with membership comprised of experts with background in the nickel-cadmium/nickel-hydrogen secondary battery/power systems areas. The work and recommendations of that subcommittee are presented.

  15. KSC-02pd0622

    NASA Image and Video Library

    2002-04-30

    KENNEDY SPACE CENTER, FLA. - At the 2002 Space Congress, Cape Canaveral, Fla., held April 30 - May 3, visitors look at astronauts' gloves worn during spacewalks. The exhibit highlighted the Hubble Space Telescope 3B Servicing Mission (STS-109) in March 2002. The Space Congress is held annually to highlight military and space initiatives, new technologies, and Florida's role in programs and research. This year's theme is Beginning a New Era - Initiatives in Space. NASA presented several paper sessions, including Hubble Discoveries and Advancements in Technology. Space Congress is sponsored by the Canaveral Council of Technical Societies

  16. A computer controlled power tool for the servicing of the Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    Richards, Paul W.; Konkel, Carl; Smith, Chris; Brown, Lee; Wagner, Ken

    1996-01-01

    The Hubble Space Telescope (HST) Pistol Grip Tool (PGT) is a self-contained, microprocessor controlled, battery-powered, 3/8-inch-drive hand-held tool. The PGT is also a non-powered ratchet wrench. This tool will be used by astronauts during Extravehicular Activity (EVA) to apply torque to the HST and HST Servicing Support Equipment mechanical interfaces and fasteners. Numerous torque, speed, and turn or angle limits are programmed into the PGT for use during various missions. Batteries are replaceable during ground operations, Intravehicular Activities, and EVA's.

  17. The Case for Interactionism in Language Processing.

    DTIC Science & Technology

    1987-04-28

    D-AIBB 133 THE CASE FOR INTERACTIONISM IN LANGUAGE PROCESSING(U) 1/1 CARNEGIE-MELLON UNIV PITTSBURGH PA DEPT OF PSYCHOLOGY J L MCCLELLAND, 28 APR 87...Interaction in Language Processing The Case for Interactionism in Language Processing James L. McClelland Department of Psychology Carnegie-Mellon...REPORT NUMBER(S) 5 MONITORING ORGANIZATION REPORT NUMBER(S) Technical Report 0NR-87-1 6a NAME OF PERFORMING ORGANIZATION 6b OFFICE SYMBOL 7a. NAME OF

  18. Looking Back, Going Forward: The Carnegie Commission Tuition Policy. The New Millennium Project on Higher Education Costs, Pricing, and Productivity Working Paper.

    ERIC Educational Resources Information Center

    Wellman, Jane V.

    In thinking about the design of public policy for higher education finance, it may be instructive to look back at the evolution of finance policy and how it has worked over the last three decades of U.S. higher education. The vehicle for this exploration is the tuition policy framework developed by the Carnegie Commission on Higher Education…

  19. A Tutorial on Techniques and Applications for Natural Language Processing

    DTIC Science & Technology

    1983-10-17

    mentioned above as specific to context-free grammars were tackled by linguists, in particular Chomsky [21, 221 through Transformational Grammar . As shown...DTIC e, C 17 October 1983 MAY 1,5 1990 DEPARTMENT of COMPUTER SCIENCE Approved for pu ]3 -- ,. " Carnegie-Mellon University . . . - -A.,,Anm m n n n n ln...A Tutorial on Techniques and Applications for Natural Language Processing Philip J. Hayes and Jaime G. Carbonell Carnegie-Mellon University 17

  20. Cultural Resources Literature Search and Records Review of the Camp Ripley, General E. A. Walsh Training Center, Morrison County, Minnesota.

    DTIC Science & Technology

    1985-07-12

    Falls; Joseph Minshaw, Little Falls; Anne Rebischke and Cheryl Seelen, Carnegie Library, Little Falls; Darwin Carlson, Charlene Starin, and Veryl E...Fort Snelling History Center, St. Paul. Cheryl Seelen, Carnegie Library, Little Falls. Jan Warner, Morrison County Historical Society, Weyerhaeuser...Enclosure Wayne A. Knott Chief, Environmental Resources Branch Planning Division o" 𔃺%~*-:\\\\~% v~~ ~* ** . **:- ~** , -108- Ki ST. PAUL DISTRICT

  1. The Carnegie Mellon University Insert Project

    DTIC Science & Technology

    1997-02-01

    Real - Time Systems (INSERT) project under the DARPA Evolutionary Design for Complex Software (EDCS) Program. The INSERT team has completed an initial API definition and ported the existing real-time publication subscription group communication software to LynxOS 2.4, a POSIX.1b compliant OS. The distributed real-time publisher/subscriber communication model is now supported by a processor membership protocol which allows a node in the system to fail, or to rejoin the system later. When a node fails, all the publishers and subscribers on that node have to be

  2. Tectonic Evolution of the Terrestrial Planets

    NASA Technical Reports Server (NTRS)

    Solomon, Sean C.; Senski, David G. (Technical Monitor)

    2002-01-01

    The NASA Planetary Geology and Geophysics Program supported a wide range of work on the geophysical evolution of the terrestrial planets during the period 1 April 1997 - 30 September 2001. We here provide highlights of the research carried out under this grant over the final year of the award, and we include a full listing of publications and scientific meeting presentations supported by this project. Throughout the grant period, our group consisted of the Principal Investigator and several Postdoctoral Associates, all at the Department of Terrestrial Magnetism (DTM) of the Carnegie Institution of Washington.

  3. The carnegie protein trap library: a versatile tool for Drosophila developmental studies.

    PubMed

    Buszczak, Michael; Paterno, Shelley; Lighthouse, Daniel; Bachman, Julia; Planck, Jamie; Owen, Stephenie; Skora, Andrew D; Nystul, Todd G; Ohlstein, Benjamin; Allen, Anna; Wilhelm, James E; Murphy, Terence D; Levis, Robert W; Matunis, Erika; Srivali, Nahathai; Hoskins, Roger A; Spradling, Allan C

    2007-03-01

    Metazoan physiology depends on intricate patterns of gene expression that remain poorly known. Using transposon mutagenesis in Drosophila, we constructed a library of 7404 protein trap and enhancer trap lines, the Carnegie collection, to facilitate gene expression mapping at single-cell resolution. By sequencing the genomic insertion sites, determining splicing patterns downstream of the enhanced green fluorescent protein (EGFP) exon, and analyzing expression patterns in the ovary and salivary gland, we found that 600-900 different genes are trapped in our collection. A core set of 244 lines trapped different identifiable protein isoforms, while insertions likely to act as GFP-enhancer traps were found in 256 additional genes. At least 8 novel genes were also identified. Our results demonstrate that the Carnegie collection will be useful as a discovery tool in diverse areas of cell and developmental biology and suggest new strategies for greatly increasing the coverage of the Drosophila proteome with protein trap insertions.

  4. Development of the MAMA Detectors for the Hubble Space Telescope Imaging Spectrograph

    NASA Technical Reports Server (NTRS)

    Timothy, J. Gethyn

    1997-01-01

    The development of the Multi-Anode Microchannel Array (MAMA) detector systems started in the early 1970's in order to produce multi-element detector arrays for use in spectrographs for solar studies from the Skylab-B mission. Development of the MAMA detectors for spectrographs on the Hubble Space Telescope (HST) began in the late 1970's, and reached its culmination with the successful installation of the Space Telescope Imaging Spectrograph (STIS) on the second HST servicing mission (STS-82 launched 11 February 1997). Under NASA Contract NAS5-29389 from December 1986 through June 1994 we supported the development of the MAMA detectors for STIS, including complementary sounding rocket and ground-based research programs. This final report describes the results of the MAMA detector development program for STIS.

  5. Using Microsoft Excel to teach statistics in a graduate advanced practice nursing program.

    PubMed

    DiMaria-Ghalili, Rose Ann; Ostrow, C Lynne

    2009-02-01

    This article describes the authors' experiences during 3 years of using Microsoft Excel to teach graduate-level statistics, as part of the research core required by the American Association of Colleges of Nursing for all professional graduate nursing programs. The advantages to using this program instead of specialized statistical programs are ease of accessibility, increased transferability of skills, and reduced cost for students. The authors share their insight about realistic goals for teaching statistics to master's-level students and the resources that are available to faculty to help them to learn and use Excel in their courses. Several online sites that are excellent resources for both faculty and students are discussed. Detailed attention is given to an online course (Carnegie-Mellon University Open Learning Initiative, n.d.), which the authors have incorporated into their graduate-level research methods course.

  6. Using Six Sigma to Accelerate the Adoption of CMMI for Optimal Results

    DTIC Science & Technology

    2004-10-01

    Findings Path forward © 2004 by Carnegie Mellon University Version 1.0 page 5 Carnegie Mellon S oftware Engineer ing Inst itute Software & IT Best...Related Technology ( COBIT ) Secondary priority • architecture best practices and Design for Six Sigma Primary audiences • Software Engineering Process Groups...itute Context of Findings While our focus was on CMMI, ITIL, and COBIT , we gathered information on other technologies “in play.” • The list included

  7. The Hubble Space Telescope: UV, Visible, and Near-Infrared Pursuits

    NASA Technical Reports Server (NTRS)

    Wiseman, Jennifer

    2010-01-01

    The Hubble Space Telescope continues to push the limits on world-class astrophysics. Cameras including the Advanced Camera for Surveys and the new panchromatic Wide Field Camera 3 which was installed nu last year's successful servicing mission S2N4,o{fer imaging from near-infrared through ultraviolet wavelengths. Spectroscopic studies of sources from black holes to exoplanet atmospheres are making great advances through the versatile use of STIS, the Space Telescope Imaging Spectrograph. The new Cosmic Origins Spectrograph, also installed last year, is the most sensitive UV spectrograph to fly io space and is uniquely suited to address particular scientific questions on galaxy halos, the intergalactic medium, and the cosmic web. With these outstanding capabilities on HST come complex needs for laboratory astrophysics support including atomic and line identification data. I will provide an overview of Hubble's current capabilities and the scientific programs and goals that particularly benefit from the studies of laboratory astrophysics.

  8. Personal renewal.

    PubMed

    Gardner, J W

    1992-10-01

    After John Gardner's presentation on "Self-Renewal" to THE WESTERN JOURNAL OF MEDICINE Editors' Meeting, (*) Joseph Murphy, MD, Special Editor for Wyoming, asked the former Secretary of Health, Education, and Welfare, "Where are you in your life's cycle?" Dr Gardner, who is 80 years old, answered, "When Chief Justice Oliver Wendell Holmes, Jr, was in his 90s, he was asked a similar question and said, ;I'm like a race horse cantering along after the race is over, cooling down.' Well, I'm nowhere near cantering! I'm still in the race, pushing the world." race, pushing the world."John Gardner, who received his undergraduate degree from Stanford and PhD from the University of California, Berkeley, taught at the college level for several years before he joined the Carnegie Foundation. As president of Carnegie Corporation and Carnegie Foundation for the Advancement of Teaching, he began to "push the world" toward education and in 1964 received the country's highest civilian honor, the Presidential Medal of Freedom. He has also pushed it toward political reform by founding Common Cause, toward grass-roots political action by founding the Urban Coalition, toward leadership training by founding the White House Fellows program, and toward volunteerism by founding the Independent Sector (a coalition of for-profit and not-for-profit organizations and foundations). His books, including Excellence, Self-Renewal, No Easy Victories, and On Leadership, have pushed readers to new understanding of themselves and of organizations to higher levels of creativity and energy to get important work done. His current research focuses on discovering and defining the characteristics of healthy, vital communities. His call to "keep on keeping on," indeed, to push the world, leads to constructive change. Active people become effective people, infused with the energy and optimism that good hard work inspires. I think you will find this paper as invigorating to read as it was to hear.

  9. New Constraints on the Faint End of the UV Luminosity Function at z ~ 7-8 Using the Gravitational Lensing of the Hubble Frontier Fields Cluster A2744

    NASA Astrophysics Data System (ADS)

    Atek, Hakim; Richard, Johan; Kneib, Jean-Paul; Jauzac, Mathilde; Schaerer, Daniel; Clement, Benjamin; Limousin, Marceau; Jullo, Eric; Natarajan, Priyamvada; Egami, Eiichi; Ebeling, Harald

    2015-02-01

    Exploiting the power of gravitational lensing, the Hubble Frontier Fields (HFF) program aims at observing six massive galaxy clusters to explore the distant universe far beyond the limits of blank field surveys. Using the complete Hubble Space Telescope observations of the first HFF cluster A2744, we report the detection of 50 galaxy candidates at z ~ 7 and eight candidates at z ~ 8 in a total survey area of 0.96 arcmin2 in the source plane. Three of these galaxies are multiply imaged by the lensing cluster. Using an updated model of the mass distribution in the cluster we were able to calculate the magnification factor and the effective survey volume for each galaxy in order to compute the ultraviolet galaxy luminosity function (LF) at both redshifts 7 and 8. Our new measurements reliably extend the z ~ 7 UV LF down to an absolute magnitude of M UV ~ -15.5. We find a characteristic magnitude of M\\star UV = -20.90+0.90-0.73 mag and a faint-end slope α =-2.01+0.20-0.28, close to previous determinations in blank fields. We show here for the first time that this slope remains steep down to very faint luminosities of 0.01 L sstarf. Although prone to large uncertainties, our results at z ~ 8 also seem to confirm a steep faint-end slope below 0.1 L sstarf. The HFF program is therefore providing an extremely efficient way to study the faintest galaxy populations at z > 7 that would otherwise be inaccessible with current instrumentation. The full sample of six galaxy clusters will provide even better constraints on the buildup of galaxies at early epochs and their contribution to cosmic reionization. Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs 13495, 11386, 13389, and 11689. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. The Hubble Frontier Fields data were obtained from the Mikulski Archive for Space Telescopes (MAST).

  10. Continuous Risk Management: A NASA Program Initiative

    NASA Technical Reports Server (NTRS)

    Hammer, Theodore F.; Rosenberg, Linda

    1999-01-01

    NPG 7120.5A, "NASA Program and Project Management Processes and Requirements" enacted in April, 1998, requires that "The program or project manager shall apply risk management principles..." The Software Assurance Technology Center (SATC) at NASA GSFC has been tasked with the responsibility for developing and teaching a systems level course for risk management that provides information on how to comply with this edict. The course was developed in conjunction with the Software Engineering Institute at Carnegie Mellon University, then tailored to the NASA systems community. This presentation will briefly discuss the six functions for risk management: (1) Identify the risks in a specific format; (2) Analyze the risk probability, impact/severity, and timeframe; (3) Plan the approach; (4) Track the risk through data compilation and analysis; (5) Control and monitor the risk; (6) Communicate and document the process and decisions.

  11. Nuclear Successor States of the Soviet Union, Nuclear Weapon and Sensitive Export Status Report

    DTIC Science & Technology

    1994-05-01

    EXPORT STATUS REPORT S I VIE T U N il] N A COOPERATIVE PROJECT OF THE CARNEGIE ENDOWMENT FOR INTERNATIONAL PEACE, WASHINGTON, DC, AND MOSCOW NUMBER 1...Launch Periodic Report on Nuclear Successor States Leonard S . Spector of the Carnegie Endowment for N U C L E A R International Peace and William C...range, translated in FBIS-SOV-92-232, December 2, 1992, p. 22. 5 Table I-C. -- N -Weapon Systems and Warheads on Territory, con’t. S

  12. Cyber Intelligence: Challenges and Best Practices

    DTIC Science & Technology

    2015-01-15

    2015 2 . REPORT TYPE N/A 3. DATES COVERED 4. TITLE AND SUBTITLE Cyber Intelligence Challenges and Best Practices 5a. CONTRACT NUMBER 5b...ANSI Std Z39-18 2 Cyber Intel – Challenges and Best Practices January 2015 © 2015 Carnegie Mellon University Copyright 2015 Carnegie Mellon University...University Reporting timelines Gov’t Agency 1 Gov’t Agency 2 Gov’t Agency 3 Gov’t Agency 4 Urgent Normal Strategic 2 -4 Hours 1 Day 1 Month 1 Day 2

  13. A TREETOPS simulation of the Hubble Space Telescope-High Gain Antenna interaction

    NASA Technical Reports Server (NTRS)

    Sharkey, John P.

    1987-01-01

    Virtually any project dealing with the control of a Large Space Structure (LSS) will involve some level of verification by digital computer simulation. While the Hubble Space Telescope might not normally be included in a discussion of LSS, it is presented to highlight a recently developed simulation and analysis program named TREETOPS. TREETOPS provides digital simulation, linearization, and control system interaction of flexible, multibody spacecraft which admit to a point-connected tree topology. The HST application of TREETOPS is intended to familiarize the LSS community with TREETOPS by presenting a user perspective of its key features.

  14. GETTING TO THE HEART OF A GALAXY

    NASA Technical Reports Server (NTRS)

    2002-01-01

    This collage of images in visible and infrared light reveals how the barred spiral galaxy NGC 1365 is feeding material into its central region, igniting massive star birth and probably causing its bulge of stars to grow. The material also is fueling a black hole in the galaxy's core. A galaxy's bulge is a central, football-shaped structure composed of stars, gas, and dust. The black-and-white image in the center, taken by a ground-based telescope, displays the entire galaxy. But the telescope's resolution is not powerful enough to reveal the flurry of activity in the galaxy's hub. The blue box in the galaxy's central region outlines the area observed by the NASA Hubble Space Telescope's visible-light camera, the Wide Field and Planetary Camera 2 (WFPC2). The red box pinpoints a narrower view taken by the Hubble telescope's infrared camera, the Near Infrared Camera and Multi-Object Spectrometer (NICMOS). A barred spiral is characterized by a lane of stars, gas, and dust slashing across a galaxy's central region. It has a small bulge that is dominated by a disk of material. The spiral arms begin at both ends of the bar. The bar is funneling material into the hub, which triggers star formation and feeds the bulge. The visible-light picture at upper left is a close-up view of the galaxy's hub. The bright yellow orb is the nucleus. The dark material surrounding the orb is gas and dust that is being funneled into the central region by the bar. The blue regions pinpoint young star clusters. In the infrared image at lower right, the Hubble telescope penetrates the dust seen in the WFPC2 picture to reveal more clusters of young stars. The bright blue dots represent young star clusters; the brightest of the red dots are young star clusters enshrouded in dust and visible only in the infrared image. The fainter red dots are older star clusters. The WFPC2 image is a composite of three filters: near-ultraviolet (3327 Angstroms), visible (5552 Angstroms), and near-infrared (8269 Angstroms). The NICMOS image, taken at a wavelength of 16,000 Angstroms, was combined with the visible and near-infrared wavelengths taken by WFPC2. The WFPC2 image was taken in January 1996; the NICMOS data were taken in April 1998. Credits for the ground-based image: Allan Sandage (The Observatories of the Carnegie Institution of Washington) and John Bedke (Computer Sciences Corporation and the Space Telescope Science Institute) Credits for the WFPC2 image: NASA and John Trauger (Jet Propulsion Laboratory) Credits for the NICMOS image: NASA, ESA, and C. Marcella Carollo (Columbia University)

  15. The Carnegie Supernova Project: The Low-Redshift Survey

    NASA Astrophysics Data System (ADS)

    Hamuy, Mario; Folatelli, Gastón; Morrell, Nidia I.; Phillips, Mark M.; Suntzeff, Nicholas B.; Persson, S. E.; Roth, Miguel; Gonzalez, Sergio; Krzeminski, Wojtek; Contreras, Carlos; Freedman, Wendy L.; Murphy, D. C.; Madore, Barry F.; Wyatt, P.; Maza, José; Filippenko, Alexei V.; Li, Weidong; Pinto, P. A.

    2006-01-01

    Supernovae are essential to understanding the chemical evolution of the universe. Type Ia supernovae also provide the most powerful observational tool currently available for studying the expansion history of the universe and the nature of dark energy. Our basic knowledge of supernovae comes from the study of their photometric and spectroscopic properties. However, the presently available data sets of optical and near-infrared light curves of supernovae are rather small and/or heterogeneous, and employ photometric systems that are poorly characterized. Similarly, there are relatively few supernovae whose spectral evolution has been well sampled, both in wavelength and phase, with precise spectrophotometric observations. The low-redshift portion of the Carnegie Supernova Project (CSP) seeks to remedy this situation by providing photometry and spectrophotometry of a large sample of supernovae taken on telescope/filter/detector systems that are well understood and well characterized. During a 5 year program that began in 2004 September, we expect to obtain high-precision u'g'r'i'BVYJHKs light curves and optical spectrophotometry for about 250 supernovae of all types. In this paper we provide a detailed description of the CSP survey observing and data reduction methodology. In addition, we present preliminary photometry and spectra obtained for a few representative supernovae during the first observing campaign.

  16. The Carnegie Protein Trap Library: A Versatile Tool for Drosophila Developmental Studies

    PubMed Central

    Buszczak, Michael; Paterno, Shelley; Lighthouse, Daniel; Bachman, Julia; Planck, Jamie; Owen, Stephenie; Skora, Andrew D.; Nystul, Todd G.; Ohlstein, Benjamin; Allen, Anna; Wilhelm, James E.; Murphy, Terence D.; Levis, Robert W.; Matunis, Erika; Srivali, Nahathai; Hoskins, Roger A.; Spradling, Allan C.

    2007-01-01

    Metazoan physiology depends on intricate patterns of gene expression that remain poorly known. Using transposon mutagenesis in Drosophila, we constructed a library of 7404 protein trap and enhancer trap lines, the Carnegie collection, to facilitate gene expression mapping at single-cell resolution. By sequencing the genomic insertion sites, determining splicing patterns downstream of the enhanced green fluorescent protein (EGFP) exon, and analyzing expression patterns in the ovary and salivary gland, we found that 600–900 different genes are trapped in our collection. A core set of 244 lines trapped different identifiable protein isoforms, while insertions likely to act as GFP-enhancer traps were found in 256 additional genes. At least 8 novel genes were also identified. Our results demonstrate that the Carnegie collection will be useful as a discovery tool in diverse areas of cell and developmental biology and suggest new strategies for greatly increasing the coverage of the Drosophila proteome with protein trap insertions. PMID:17194782

  17. A Striking Perspective

    NASA Image and Video Library

    2015-04-16

    This image from NASA MESSENGER spacecraft provides a perspective view of the center portion of Carnegie Rupes, a large tectonic landform, which cuts through Duccio crater. The image shows the terrain (variations in topography) as measured by the MLA instrument and surface mapped by the MDIS instrument. The image was color-coded to highlight the variations in topography (red = high standing terrain, blue = low lying terrain). Tectonic landforms such as Carnegie Rupes form on Mercury as a response to interior planetary cooling, resulting in the overall shrinking of the planet. To make this graphic, 48 individual MDIS images were used as part of the mosaic. Instruments: Mercury Dual Imaging System (MDIS) and Mercury Laser Altimeter (MLA) Latitude: 57.1° Longitude: 304.0° E Scale: Duccio crater has a diameter of roughly 105 kilometers (65 miles) Height: Portions of Carnegie Rupes are nearly 2 kilometers (1.2 miles) in height Orientation: North is roughly to the left of the image http://photojournal.jpl.nasa.gov/catalog/PIA19422

  18. STS-103 perfect night-time landing for Space Shuttle Discovery

    NASA Technical Reports Server (NTRS)

    1999-01-01

    The orbiter Discovery looks like a blue ghost as it drops from the darkness onto lighted runway 33 at KSC's Shuttle Landing Facility. After traveling more than 3,267,000 miles on a successful eight-day mission to service the Hubble Space Telescope, the orbiter touches down at 7:00:47 p.m. EST. Aboard are Commander Curtis L. Brown Jr., Pilot Scott J. Kelly, and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.), Claude Nicollier of Switzerland and Jean-Frangois Clervoy of France, who spent the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history.

  19. KSC-99pp1511

    NASA Image and Video Library

    1999-12-27

    KENNEDY SPACE CENTER, Fla. -- The orbiter Discovery looks like a blue ghost as it drops from the darkness onto lighted runway 33 at KSC's Shuttle Landing Facility. After traveling more than 3,267,000 miles on a successful eight-day mission to service the Hubble Space Telescope, the orbiter touches down at 7:00:47 p.m. EST. Aboard are Commander Curtis L. Brown Jr., Pilot Scott J. Kelly, and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.), Claude Nicollier of Switzerland and Jean-François Clervoy of France, who spent the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  20. Human Space Flight Plans Committee

    NASA Image and Video Library

    2009-06-16

    U.S. Sen. Bill Nelson, D-Fla., at podium, addresses members of the Human Space Flight Review Committee, Wednesday, June 17, 2009, at the Carnegie Institution in Washington. Seated from left are Jeffrey Greason, Bohdan Bejmuk, Dr. Leroy Chiao, Norman Augustine (chair), Dr. Wanda Austin, Dr. Edward Crawley, Dr. Christopher Chyba and Philip McAlister. The panel will examine ongoing and planned NASA development activities and potential alternatives in order to present options for advancing a safe, innovative, affordable and sustainable human space flight program following the space shuttle's retirement. The committee wil present its results by August 2009. Photo Credit: (NASA/Paul E. Alers)

  1. The Great Observatories Origins Deep Survey (GOODS): Overview and Status

    NASA Astrophysics Data System (ADS)

    Hook, R. N.; GOODS Team

    2002-12-01

    GOODS is a very large project to gather deep imaging data and spectroscopic followup of two fields, the Hubble Deep Field North (HDF-N) and the Chandra Deep Field South (CDF-S), with both space and ground-based instruments to create an extensive multiwavelength public data set for community research on the distant Universe. GOODS includes a SIRTF Legacy Program (PI: Mark Dickinson) and a Hubble Treasury Program of ACS imaging (PI: Mauro Giavalisco). The ACS imaging was also optimized for the detection of high-z supernovae which are being followed up by a further target of opportunity Hubble GO Program (PI: Adam Riess). The bulk of the CDF-S ground-based data presently available comes from an ESO Large Programme (PI: Catherine Cesarsky) which includes both deep imaging and multi-object followup spectroscopy. This is currently complemented in the South by additional CTIO imaging. Currently available HDF-N ground-based data forming part of GOODS includes NOAO imaging. Although the SIRTF part of the survey will not begin until later in the year the ACS imaging is well advanced and there is also a huge body of complementary ground-based imaging and some follow-up spectroscopy which is already publicly available. We summarize the current status of GOODS and give an overview of the data products currently available and present the timescales for the future. Many early science results from the survey are presented in other GOODS papers at this meeting. Support for the HST GOODS program presented here and in companion abstracts was provided by NASA thorugh grant number GO-9425 from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.

  2. Twenty-Three High-Redshift Supernovae from the Institute for Astronomy Deep Survey: Doubling the Supernova Sample at z > 0.7

    NASA Astrophysics Data System (ADS)

    Barris, Brian J.; Tonry, John L.; Blondin, Stéphane; Challis, Peter; Chornock, Ryan; Clocchiatti, Alejandro; Filippenko, Alexei V.; Garnavich, Peter; Holland, Stephen T.; Jha, Saurabh; Kirshner, Robert P.; Krisciunas, Kevin; Leibundgut, Bruno; Li, Weidong; Matheson, Thomas; Miknaitis, Gajus; Riess, Adam G.; Schmidt, Brian P.; Smith, R. Chris; Sollerman, Jesper; Spyromilio, Jason; Stubbs, Christopher W.; Suntzeff, Nicholas B.; Aussel, Hervé; Chambers, K. C.; Connelley, M. S.; Donovan, D.; Henry, J. Patrick; Kaiser, Nick; Liu, Michael C.; Martín, Eduardo L.; Wainscoat, Richard J.

    2004-02-01

    We present photometric and spectroscopic observations of 23 high-redshift supernovae (SNe) spanning a range of z=0.34-1.03, nine of which are unambiguously classified as Type Ia. These SNe were discovered during the IfA Deep Survey, which began in 2001 September and observed a total of 2.5 deg2 to a depth of approximately m~25-26 in RIZ over 9-17 visits, typically every 1-3 weeks for nearly 5 months, with additional observations continuing until 2002 April. We give a brief description of the survey motivations, observational strategy, and reduction process. This sample of 23 high-redshift SNe includes 15 at z>=0.7, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry et al. (2003), we calculate cosmological parameter density contours that are consistent with the flat universe indicated by the cosmic microwave background (Spergel et al. 2003). Adopting the constraint that Ωtotal=1.0, we obtain best-fit values of (Ωm,ΩΛ)=(0.33,0.67) using 22 SNe from this survey augmented by the literature compilation. We show that using the empty-beam model for gravitational lensing does not eliminate the need for ΩΛ>0. Experience from this survey indicates great potential for similar large-scale surveys while also revealing the limitations of performing surveys for z>1 SNe from the ground. CFHT: Based in part on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. CTIO: Based in part on observations taken at the Cerro Tololo Inter-American Observatory. Keck: Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Magellan: Based in part on observations from the 6.5 m Baade telescope operated by the Observatories of the Carnegie Institution of Washington for the Magellan Consortium, a collaboration between the Carnegie Observatories, the University of Arizona, Harvard University, the University of Michigan, and the Massachusetts Institute of Technology. UH: Based in part on observations with the University of Hawaii 2.2 m telescope at Mauna Kea Observatory, Institute for Astronomy, University of Hawaii. VLT: Based in part on observations obtained at the European Southern Observatory, Paranal, Chile, under programs ESO 68.A-0427. Based in part on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS5-26555. This research is primarily associated with proposal GO-09118.

  3. Aerospace applications of virtual environment technology.

    PubMed

    Loftin, R B

    1996-11-01

    The uses of virtual environment technology in the space program are examined with emphasis on training for the Hubble Space Telescope Repair and Maintenance Mission in 1993. Project ScienceSpace at the Virtual Environment Technology Lab is discussed.

  4. The future of space imaging. Report of a community-based study of an advanced camera for the Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    Brown, Robert A. (Editor)

    1993-01-01

    The scientific and technical basis for an Advanced Camera (AC) for the Hubble Space Telescope (HST) is discussed. In March 1992, the NASA Program Scientist for HST invited the Space Telescope Science Institute to conduct a community-based study of an AC, which would be installed on a scheduled HST servicing mission in 1999. The study had three phases: a broad community survey of views on candidate science program and required performance of the AC, an analysis of technical issues relating to its implementation, and a panel of experts to formulate conclusions and prioritize recommendations. From the assessment of the imaging tasks astronomers have proposed for or desired from HST, we believe the most valuable 1999 instrument would be a camera with both near ultraviolet/optical (NUVO) and far ultraviolet (FUV) sensitivity, and with both wide field and high resolution options.

  5. Lake Carnegie, Western Australia

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Ephemeral Lake Carnegie, in Western Australia, fills with water only during periods of significant rainfall. In dry years, it is reduced to a muddy marsh. This image was acquired by Landsat 7's Enhanced Thematic Mapper plus (ETM+) sensor on May 19, 1999. This is a false-color composite image made using shortwave infrared, infrared, and red wavelengths. The image has also been sharpened using the sensor's panchromatic band. Image provided by the USGS EROS Data Center Satellite Systems Branch. This image is part of the ongoing Landsat Earth as Art series.

  6. A Tutorial for Building CMMI Process Performance Models

    DTIC Science & Technology

    2010-04-26

    70 90 120 1 0~-----0~----~ 2 Arch itecture/ Design All New Code M ajor Reuse of Code 55 70 90 8 10 15 2 0~-----0~----~ 3 Code All New Code M ajor...Robert Stoddard and Dave Zubrow © 2010 Carnegie Mellon University t "’ ·=··=· "’ •• ,. ...... ,. .... ~ .00 1 Arch [’ <si!JI ~h~;,...o ’ .. CodeChoice...Carnegie Mellon University : • Fit Model It; b][g~ El Model Select Columns 41111Delivered0efect; 411111nspection0 efect ..ollllnspectionCover

  7. A Sneak Peek at the JWST Era: Observing Galaxies Below the Hubble Limit with Gravitational Lensing

    NASA Astrophysics Data System (ADS)

    Livermore, Rachael C.

    2016-01-01

    The installation of WFC3 on the Hubble Space Telescope pushed the frontier of high-redshift galaxy studies to only 500 Myr after the Big Bang. However, observations in this epoch remain challenging and are limited to the brightest galaxies; the fainter sources believed to be responsible for reionizing the Universe remain beyond the grasp of Hubble. With gravitational lensing, however, we can benefit from the magnification of faint sources, which brings them within reach of today's telescopes. The Hubble Frontier Fields program is a deep survey of strongly lensing clusters observed in the optical and near-infrared. Unfortunately, detecting highly magnified, intrinsically faint galaxies in these fields has proved challenging due to the bright foregound cluster galaxies and intracluster light. We have developed a technique using wavelet decomposition to overcome these difficulties and detect galaxies at z~7 with intrinsic UV magnitudes as faint as MUV = -13. We present this method and the resulting luminosity functions, which support a steep faint-end slope extending out to the observational limits. Our method has uncovered hundreds of galaxies at z > 6 fainter than any that have been seen before, providing our first insight into the small galaxy population during the epoch of reionization and a preview of the capabilities of JWST.

  8. The Hubble Space Telescope's Student ERO Pilot Project: Implementing Formal and Informal Collaborative Projects

    NASA Astrophysics Data System (ADS)

    Eisenhamer, Bonnie; Ryer, H.; McCallister, D.; Taylor, J.; Bishop, M.

    2010-05-01

    The Hubble Space Telescope's Early Release Observations (EROs) were revealed to the public on September 9, 2009, and K-12 students and educators in six states across the country are joining in the celebration. Students and educators in Maryland, Ohio, New York, California, New Mexico, and Delaware have been invited to participate in the Hubble Space Telescope's Student ERO Pilot Project. This is an interdisciplinary project created by STScI's Office of Public Outreach in which students research the four ERO objects and create various types of projects. In recognition of their participation, the projects are displayed at host institutions in each state (museum, science center, school, planetarium or library) during a special public event for participating students, their families, and teachers. As part of its evaluation program, STScI's Office of Public Outreach has been conducting an evaluation of the project to determine the viability and potential of conducting large-scale, formal/informal collaborative projects in the future. This poster will highlight preliminary findings and share lessons learned.

  9. The Lick-Carnegie Exoplanet Survey: A Saturn-Mass Planet in the Habitable Zone of the Nearby M4V Star HIP 57050

    NASA Astrophysics Data System (ADS)

    Haghighipour, Nader; Vogt, Steven S.; Butler, R. Paul; Rivera, Eugenio J.; Laughlin, Greg; Meschiari, Stefano; Henry, Gregory W.

    2010-05-01

    Precision radial velocities (RV) from Keck/HIRES reveal a Saturn-mass planet orbiting the nearby M4V star HIP 57050. The planet has a minimum mass of Msin i ~ 0.3 M J, an orbital period of 41.4 days, and an orbital eccentricity of 0.31. V-band photometry reveals a clear stellar rotation signature of the host star with a period of 98 days, well separated from the period of the RV variations and reinforcing a Keplerian origin for the observed velocity variations. The orbital period of this planet corresponds to an orbit in the habitable zone of HIP 57050, with an expected planetary temperature of ~230 K. The star has a metallicity of [Fe/H] = 0.32 ± 0.06 dex, of order twice solar and among the highest metallicity stars in the immediate solar neighborhood. This newly discovered planet provides further support that the well-known planet-metallicity correlation for F, G, and K stars also extends down into the M-dwarf regime. The a priori geometric probability for transits of this planet is only about 1%. However, the expected eclipse depth is ~7%, considerably larger than that yet observed for any transiting planet. Though long on the odds, such a transit is worth pursuing as it would allow for high quality studies of the atmosphere via transmission spectroscopy with Hubble Space Telescope. At the expected planetary effective temperature, the atmosphere may contain water clouds.

  10. JWST Program Implementation

    NASA Astrophysics Data System (ADS)

    Januszewski, William

    2018-01-01

    This poster will feature what is involved in preparing a James Webb Space Telescope program for execution on board the spacecraft. The process from when the principle investigator hits the submit button to when the observations are executed on board the spacecraft will be addressed. Although the process shares a number of sumilarities with the implementation process for the Hubble Space Telescope, there are significant differences.

  11. Translating the Birmingham Neighborhood Leaders Survey into Innovative Action through the Community Health Innovation Awards.

    PubMed

    Allen, Shauntice; Pineda, Alaina; Hood, Anthony C; Wakelee, Jessica F

    2017-01-01

    The Carnegie Foundation for the Advancement of Teaching describes community engagement as the collaboration between higher education institutions and their larger communities (local, regional/state, national, global) for the mutually beneficial exchange of knowledge and resources in a context of partnership. This article describes the development, implementation and outcomes of a community-engaged grant-making program, the Community Health Innovation Awards (CHIA). The CHIA program was the by-product of a qualitative study jointly led by researchers at the University of Alabama at Birmingham and neighborhood leaders from the surrounding communities in Birmingham, AL. The competitive program provided funding to area organizations that proposed creative solutions to on-the-ground health challenges. Since its inception, CHIA has awarded $356,500 to 26 innovative projects between 2012 and 2017. These awards have supported novel programs that have connected academic and community partners in addressing health disparities and improving overall community well-being in the greater Birmingham area.

  12. VPython: Writing Real-time 3D Physics Programs

    NASA Astrophysics Data System (ADS)

    Chabay, Ruth

    2001-06-01

    VPython (http://cil.andrew.cmu.edu/projects/visual) combines the Python programming language with an innovative 3D graphics module called Visual, developed by David Scherer. Designed to make 3D physics simulations accessible to novice programmers, VPython allows the programmer to write a purely computational program without any graphics code, and produces an interactive realtime 3D graphical display. In a program 3D objects are created and their positions modified by computational algorithms. Running in a separate thread, the Visual module monitors the positions of these objects and renders them many times per second. Using the mouse, one can zoom and rotate to navigate through the scene. After one hour of instruction, students in an introductory physics course at Carnegie Mellon University, including those who have never programmed before, write programs in VPython to model the behavior of physical systems and to visualize fields in 3D. The Numeric array processing module allows the construction of more sophisticated simulations and models as well. VPython is free and open source. The Visual module is based on OpenGL, and runs on Windows, Linux, and Macintosh.

  13. Program Facilitates CMMI Appraisals

    NASA Technical Reports Server (NTRS)

    Sweetser, Wesley

    2005-01-01

    A computer program has been written to facilitate appraisals according to the methodology of Capability Maturity Model Integration (CMMI). [CMMI is a government/industry standard, maintained by the Software Engineering Institute at Carnegie Mellon University, for objectively assessing the engineering capability and maturity of an organization (especially, an organization that produces software)]. The program assists in preparation for a CMMI appraisal by providing drop-down lists suggesting required artifacts or evidence. It identifies process areas for which similar evidence is required and includes a copy feature that reduces or eliminates repetitive data entry. It generates reports to show the entire framework for reference, the appraisal artifacts to determine readiness for an appraisal, and lists of interviewees and questions to ask them during the appraisal. During an appraisal, the program provides screens for entering observations and ratings, and reviewing evidence provided thus far. Findings concerning strengths and weaknesses can be exported for use in a report or a graphical presentation. The program generates a chart showing capability level ratings of the organization. A context-sensitive Windows help system enables a novice to use the program and learn about the CMMI appraisal process.

  14. KSC-99pp1509

    NASA Image and Video Library

    1999-12-27

    After landing at the Shuttle Landing Facility, STS-103 Pilot Scott J. Kelly (left) and Commander Curtis L. Brown Jr. (right) look at the tiles on orbiter Discovery. They and other crew members Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.), Jean-Francois Clervoy of France and Claude Nicollier of Switzerland, completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  15. KSC-99pp1510

    NASA Image and Video Library

    1999-12-27

    After landing at the Shuttle Landing Facility, the STS-103 crew poses in front of the orbiter Discovery. Standing left to right are Commander Curtis L. Brown Jr., Mission Specialist Claude Nicollier of Switzerland, Pilot Scott J. Kelly, and Mission Specialists Jean-Francois Clervoy of France, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.) and Steven L. Smith. The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  16. KSC-99pp1505

    NASA Image and Video Library

    1999-12-27

    After landing at the Shuttle Landing Facility, STS-103 Mission Specialist Jean-François Clervoy of France (left), with the European Space Agency (ESA), and Commander Curtis L. Brown Jr. (right) look over the orbiter Discovery. They and other crew members Pilot Scott J. Kelly and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.) and Claude Nicollier of Switzerland (also with ESA), completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  17. KSC-99pp1504

    NASA Image and Video Library

    1999-12-27

    KENNEDY SPACE CENTER, Fla. -- The Space Shuttle Discovery drops out of the darkness onto runway 33 at the Shuttle Landing Facility after traveling more than 3,267,000 miles on a successful eight-day mission to service the Hubble Space Telescope. Astronauts Curtis L. Brown Jr., Commander; Scott J. Kelly, Pilot; and Steven L. Smith, C. Michael Foale (Ph.D.), John M. Grunsfeld (Ph.D.), Claude Nicollier of Switzerland and Jean-François Clervoy of France, all Mission Specialists, spent the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  18. Discovery and Characterization of Gravitationally Lensed X-ray Sources in the CLASH Sample

    NASA Astrophysics Data System (ADS)

    Pasha, Imad; Van Weeren, Reinout J.; Santos, Felipe A.

    2017-01-01

    We present the discovery of ~20 gravitationally lensed X-ray sources in the Cluster Lensing And Supernova survey with Hubble (CLASH) survey, a sample of massive clusters of galaxies between z ~ 0.2-0.9 observed with the Hubble Space Telescope (HST). By combining CLASH imaging with Chandra X-ray Observatory observations of the same clusters, we select those sources in the HST images which are gravitationally lensed X-ray sources behind the clusters. Of those discovered sources, we determine various properties including source redshifts and magnifications, as well as performing X-ray spectral fits to determine source fluxes and luminosities. Prior to this study, only four lensed X-ray sources behind clusters have been found, thus to the best of our knowledge, our program is the first to systematically categorize lensed X-ray sources behind galaxy clusters.This work was supported by the SAO REU program, which is funded in part by the National Science Foundation REU and Department of Defense ASSURE programs under NSF Grant no. 1262851, and by the Smithsonian Institution.

  19. Astronaut Anna Fisher Suiting Up For NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  20. Astronaut Anna Fisher Suited Up For NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suited up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  1. Astronaut Anna Fisher Suited Up For NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall SPace Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suited up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  2. Astronaut Anna Fisher Suits Up for NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  3. Astronaut Anna Fisher Suiting Up For NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. MSFC's Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  4. Astronaut Anna Fisher Suits Up For NBS Training

    NASA Technical Reports Server (NTRS)

    1980-01-01

    The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center's (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.

  5. The Carnegie Supernova Project I. Photometry data release of low-redshift stripped-envelope supernovae

    NASA Astrophysics Data System (ADS)

    Stritzinger, M. D.; Anderson, J. P.; Contreras, C.; Heinrich-Josties, E.; Morrell, N.; Phillips, M. M.; Anais, J.; Boldt, L.; Busta, L.; Burns, C. R.; Campillay, A.; Corco, C.; Castellon, S.; Folatelli, G.; González, C.; Holmbo, S.; Hsiao, E. Y.; Krzeminski, W.; Salgado, F.; Serón, J.; Torres-Robledo, S.; Freedman, W. L.; Hamuy, M.; Krisciunas, K.; Madore, B. F.; Persson, S. E.; Roth, M.; Suntzeff, N. B.; Taddia, F.; Li, W.; Filippenko, A. V.

    2018-02-01

    The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in this paper is the CSP-I photometric data release of low-redshift stripped-envelope core-collapse supernovae. The data consist of optical (uBgVri) photometry of 34 objects, with a subset of 26 having near-infrared (YJH) photometry. Twenty objects have optical pre-maximum coverage with a subset of 12 beginning at least five days prior to the epoch of B-band maximum brightness. In the near-infrared, 17 objects have pre-maximum observations with a subset of 14 beginning at least five days prior to the epoch of J-band maximum brightness. Analysis of this photometric data release is presented in companion papers focusing on techniques to estimate host-galaxy extinction and the light-curve and progenitor star properties of the sample. The analysis of an accompanying visual-wavelength spectroscopy sample of 150 spectra will be the subject of a future paper. Based on observations collected at Las Campanas Observatory.Tables 2-8 are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/609/A134

  6. Artificial intelligence in astronomy - a forecast.

    NASA Astrophysics Data System (ADS)

    Adorf, H. M.

    Since several years artificial intelligence techniques are being actively used in astronomy, particularly within the Hubble Space Telescope project. This contribution reviews achievements, analyses some problems of using artificial intelligence in an astronomical environment, and projects current AI programming trends into the future.

  7. Engineering Safety- and Security-Related Requirements for Software-Intensive Systems

    DTIC Science & Technology

    2007-02-27

    the Zoo Loop Line to enter the inner Great Apes and Monkeys taxi station. Exiting the taxi when the doors open, they head down the elevator and...Carnegie Mellon University Example Overview Very Large New Zoo Zoo Automated Taxi System (ZATS) Example Zoo Habitat Guideway Layout ZATS Context Diagram...Firesmith, 27 February 2007 © 2007 Carnegie Mellon University Very Large New Zoo P a rk in g L o ts Z o o B a c k L o ts R e s ta u ra n ts a n d S h o

  8. Human Space Flight Plans Committee

    NASA Image and Video Library

    2009-06-16

    Douglas R. Cooke, Associate Administrator for Exploration Systems Mission Directorate, at podium, addresses the Human Space Flight Review Committee, Wednesday, June 17, 2009, at the Carnegie Institution in Washington. The panel will examine ongoing and planned NASA development activities and potential alternatives in order to present options for advancing a safe, innovative, affordable and sustainable human space flight program following the space shuttle's retirement. The committee wil present its results by August 2009. Seated from left on the panel is Jeffrey Greason, Bohdan Bejmuk, Dr. Leroy Chiao, Norman Augustine (chair), Dr. Wanda Austin, Dr. Edward Crawley, Dr. Christopher Chyba and Philip McAlister. Photo Credit: (NASA/Paul E. Alers)

  9. Workshop on Mercury: Space Environment, Surface, and Interior

    NASA Technical Reports Server (NTRS)

    2001-01-01

    This volume contains abstracts that have been accepted for presentation at the Workshop on Mercury: Space Environment, Surface, and Interior, October 4-5, 2001. The Scientific Organizing Committee consisted of Mark Robinson (Northwestern University), Marty Slade (Jet Propulsion Laboratory), Jim Slavin (NASA Goddard Space Flight Center), Sean Solomon (Carnegie Institution), Ann Sprague (University of Arizona), Paul Spudis (Lunar and Planetary Institute), G. Jeffrey Taylor (University of Hawai'i), Faith Vilas (NASA Johnson Space Center), Meenakshi Wadhwa (The Field Museum), and Thomas Watters (National Air and Space Museum). Logistics, administrative, and publications support were provided by the Publications and Program Services Departments of the Lunar and Planetary Institute.

  10. Hubble's diagram and cosmic expansion

    PubMed Central

    Kirshner, Robert P.

    2004-01-01

    Edwin Hubble's classic article on the expanding universe appeared in PNAS in 1929 [Hubble, E. P. (1929) Proc. Natl. Acad. Sci. USA 15, 168–173]. The chief result, that a galaxy's distance is proportional to its redshift, is so well known and so deeply embedded into the language of astronomy through the Hubble diagram, the Hubble constant, Hubble's Law, and the Hubble time, that the article itself is rarely referenced. Even though Hubble's distances have a large systematic error, Hubble's velocities come chiefly from Vesto Melvin Slipher, and the interpretation in terms of the de Sitter effect is out of the mainstream of modern cosmology, this article opened the way to investigation of the expanding, evolving, and accelerating universe that engages today's burgeoning field of cosmology. PMID:14695886

  11. The Hubble Space Telescope Scientific Instruments

    NASA Technical Reports Server (NTRS)

    Moore, J. V.

    1986-01-01

    The paper describes the status of the five Scientific Instruments (SI's) to be flown on the Hubble Space Telescope (HST) which is planned to be launched by the Space Transportation System in the last half of 1986. Concentration is on the testing experience for each of the instruments both at the instrument level and in conjunction with the other instruments and subsystems of the HST. Since the Acceptance/Flight Qualification Program of the HST is currently underway a description of the test and verification plans to be accomplished prior to shipment to the Kennedy Space Center (KSC) and pre-launch tests plans prior to launch are provided. The paper concludes with a brief description of anticipated orbital performance.

  12. Hubble Space Telescope faint object camera instrument handbook (Post-COSTAR), version 5.0

    NASA Technical Reports Server (NTRS)

    Nota, A. (Editor); Jedrzejewski, R. (Editor); Greenfield, P. (Editor); Hack, W. (Editor)

    1994-01-01

    The faint object camera (FOC) is a long-focal-ratio, photon-counting device capable of taking high-resolution two-dimensional images of the sky up to 14 by 14 arc seconds squared in size with pixel dimensions as small as 0.014 by 0.014 arc seconds squared in the 1150 to 6500 A wavelength range. Its performance approaches that of an ideal imaging system at low light levels. The FOC is the only instrument on board the Hubble Space Telescope (HST) to fully use the spatial resolution capabilities of the optical telescope assembly (OTA) and is one of the European Space Agency's contributions to the HST program.

  13. A natural language query system for Hubble Space Telescope proposal selection

    NASA Technical Reports Server (NTRS)

    Hornick, Thomas; Cohen, William; Miller, Glenn

    1987-01-01

    The proposal selection process for the Hubble Space Telescope is assisted by a robust and easy to use query program (TACOS). The system parses an English subset language sentence regardless of the order of the keyword phases, allowing the user a greater flexibility than a standard command query language. Capabilities for macro and procedure definition are also integrated. The system was designed for flexibility in both use and maintenance. In addition, TACOS can be applied to any knowledge domain that can be expressed in terms of a single reaction. The system was implemented mostly in Common LISP. The TACOS design is described in detail, with particular attention given to the implementation methods of sentence processing.

  14. Summary of the COS Cycle 22 Calibration Program

    NASA Astrophysics Data System (ADS)

    Sonnentrucker, Paule; Becker, George; Bostroem, Azalee; Debes, John H.; Ely, Justin; Fox, Andrew; Lockwood, Sean; Oliveira, Cristina; Penton, Steven; Proffitt, Charles; Roman-Duval, Julia; Sahnow, David; Sana, Hugues; Taylor, Jo; Welty, Alan D.; Wheeler, Thomas

    2016-09-01

    We summarize the calibration activities for the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope during Cycle 22 which ran from November 2014 through October 2015. We give an overview of the COS calibration plan, COS usage statistics and we briefly describe major changes with respect to the previous cycle. High-level executive summaries for each calibration program comprising Cycle 22 are also given here. Results of the analysis attached to each program are published in separate ISRs.

  15. GSFC_20171019_m12750_HSTMessier

    NASA Image and Video Library

    2017-10-19

    This is a recording from Goddard Facebook Live Event on October 19, 2017, promoting the Hubble Messier Catalog for amateur astronomers. Hosting is Erin Kisliuk with Michelle Thaller and Kevin Hartnett as talents. Download this program in multiple formats at: http://svs.gsfc.nasa.gov/12750

  16. HST and ground-based observations of bright storms on Uranus during 2014-2015.

    NASA Astrophysics Data System (ADS)

    Sayanagi, K. M.; Sromovsky, L. A.; Fry, P. M.; De Pater, I.; Hammel, H. B.; Rages, K. A.; Baranec, C.; Delcroix, M.; Wesley, A.; Hueso, R.; Sanchez-Lavega, A.; Simon, A. A.; Wong, M. H.; Orton, G. S.; Irwin, P. G.

    2015-12-01

    We report the temporal evolution of bright, long-lived cloud features on Uranus. We observed and tracked the features between August 2014 and January 2015 with the Hubble Space Telescope, the Keck 2 10-m telescope, VLT, Gran Telescopio Canarias, Gemini, William Herschel Telescope, Robo-AO, Pic du Midi 1-m telescope, and multiple smaller telescopes operated by amateur astronomers. Surprisingly bright features were first revealed in the Keck adaptive-optics images in August; this initial set of observations motivated follow-up observations around the world. One of the storms (identified as "Feature F" in Sromovsky et al. 2015, and Feature 2 in de Pater et al. 2015), which was the deepest in that dataset, was bright enough that it was detected by multiple amateur observers, permitting us to trigger a Hubble Target of Opportunity (ToO) observation on October 14th, 2014. A complex of features at this latitude was also observed by Hubble as part of the Outer Planet Atmospheres Legacy (OPAL) program on November 8-9, 2014. We will present the temporal evolution of the cloud activities from August 2014 through January 2015, and analyze the vertical structure of the cloud features in the Hubble datasets. The Hubble images used in our study were collected with support of HST grants GO13712 to KMS and GO13937 to AAS. Sromovsky et al. 2015, "High S/N Keck and Gemini AO imaging of Uranus during 2012-2014: New cloud patterns, increasing activity, and improved wind measurements." Icarus 258, 192-223. de Pater et al. 2014, "Record-breaking storm activity on Uranus in 2014." Icarus 252, 121-128

  17. Near-infrared Detection of WD 0806-661 B with the Hubble Space Telescope

    NASA Astrophysics Data System (ADS)

    Luhman, K. L.; Morley, C. V.; Burgasser, A. J.; Esplin, T. L.; Bochanski, J. J.

    2014-10-01

    WD 0806-661 B is one of the coldest known brown dwarfs (T eff = 300-345 K) based on previous mid-infrared photometry from the Spitzer Space Telescope. In addition, it is a benchmark for testing theoretical models of brown dwarfs because its age and distance are well constrained via its primary star (2 ± 0.5 Gyr, 19.2 ± 0.6 pc). We present the first near-infrared detection of this object, which has been achieved through F110W imaging (~Y + J) with the Wide Field Camera 3 on board the Hubble Space Telescope. We measure a Vega magnitude of m 110 = 25.70 ± 0.08, which implies J ~ 25.0. When combined with the Spitzer photometry, our estimate of J helps to better define the empirical sequence of the coldest brown dwarfs in M 4.5 versus J - [4.5]. The positions of WD 0806-661 B and other Y dwarfs in that diagram are best matched by the cloudy models of Burrows et al. and the cloudless models of Saumon et al., both of which employ chemical equilibrium. The calculations by Morley et al. for 50% cloud coverage differ only modestly from the data. Spectroscopy would enable a more stringent test of the models, but based on our F110W measurement, such observations are currently possible only with Hubble, and would require at least ~10 orbits to reach a signal-to-noise ratio of ~5. Based on observations made with the NASA/ESA Hubble Space Telescope through program 12815, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555, and observations with the ESO Telescopes at Paranal Observatory under programs ID 089.C-0428 and ID 089.C-0597.

  18. UV/Visible Telescope with Hubble Disposal

    NASA Technical Reports Server (NTRS)

    Benford, Dominic J.

    2013-01-01

    Submission Overview: Our primary objective is to convey a sense of the significant advances possible in astrophysics investigations for major Cosmic Origins COR program goals with a 2.4m telescope asset outfitted with one or more advanced UV visible instruments. Several compelling science objectives were identified based on community meetings these science objectives drove the conceptual design of instruments studied by the COR Program Office during July September 2012. This RFI submission encapsulates the results of that study, and suggests that a more detailed look into the instrument suite should be conducted to prove viability and affordability to support the demonstrated scientific value. This study was conducted in the context of a larger effort to consider the options available for a mission to dispose safely of Hubble hence, the overall architecture considered for the mission we studied for the 2.4m telescope asset included resource sharing. This mitigates combined cost and risk and provides naturally for a continued US leadership role in astrophysics with an advanced, general-purpose UV visible space telescope.

  19. Developmental anatomy of the liver from computerized three-dimensional reconstructions of four human embryos (from Carnegie stage 14 to 23).

    PubMed

    Lhuaire, Martin; Tonnelet, Romain; Renard, Yohann; Piardi, Tullio; Sommacale, Daniele; Duparc, Fabrice; Braun, Marc; Labrousse, Marc

    2015-07-01

    Some aspects of human embryogenesis and organogenesis remain unclear, especially concerning the development of the liver and its vasculature. The purpose of this study was to investigate, from a descriptive standpoint, the evolutionary morphogenesis of the human liver and its vasculature by computerized three-dimensional reconstructions of human embryos. Serial histological sections of four human embryos at successive stages of development belonging to three prestigious French historical collections were digitized and reconstructed in 3D using software commonly used in medical radiology. Manual segmentation of the hepatic anatomical regions of interest was performed section by section. In this study, human liver organogenesis was examined at Carnegie stages 14, 18, 21 and 23. Using a descriptive and an analytical method, we showed that these stages correspond to the implementation of the large hepatic vascular patterns (the portal system, the hepatic artery and the hepatic venous system) and the biliary system. To our knowledge, our work is the first descriptive morphological study using 3D computerized reconstructions from serial histological sections of the embryonic development of the human liver between Carnegie stages 14 and 23. Copyright © 2015 Elsevier GmbH. All rights reserved.

  20. STS-103 crew looks over Discovery after a night-time landing at the SLF

    NASA Technical Reports Server (NTRS)

    1999-01-01

    After landing at the Shuttle Landing Facility, the STS-103 crew looks over the orbiter Discovery. In the foreground, from left, are Mission Specialist Jean-Francois Clervoy of France, Pilot Scott J. Kelly, Commander Curtis L. Brown Jr. and Mission Specialist C. Michael Foale (Ph.D.); behind them, from left, are Mission Specialists Steven L. Smith and Claude Nicollier of Switzerland. The remaining crew member (not shown) is Mission Specialist John M. Grunsfeld (Ph.D.). The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 EST and wheel stop at 7:01:34 EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history.

  1. A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 IN HUBBLE SPACE TELESCOPE INFRARED OBSERVATIONS FROM CANDELS

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Rodney, Steven A.; Riess, Adam G.; Jones, David O.

    2012-02-10

    We report the discovery of a Type Ia supernova (SN Ia) at redshift z = 1.55 with the infrared detector of the Wide Field Camera 3 (WFC3-IR) on the Hubble Space Telescope (HST). This object was discovered in CANDELS imaging data of the Hubble Ultra Deep Field and followed as part of the CANDELS+CLASH Supernova project, comprising the SN search components from those two HST multi-cycle treasury programs. This is the highest redshift SN Ia with direct spectroscopic evidence for classification. It is also the first SN Ia at z > 1 found and followed in the infrared, providing amore » full light curve in rest-frame optical bands. The classification and redshift are securely defined from a combination of multi-band and multi-epoch photometry of the SN, ground-based spectroscopy of the host galaxy, and WFC3-IR grism spectroscopy of both the SN and host. This object is the first of a projected sample at z > 1.5 that will be discovered by the CANDELS and CLASH programs. The full CANDELS+CLASH SN Ia sample will enable unique tests for evolutionary effects that could arise due to differences in SN Ia progenitor systems as a function of redshift. This high-z sample will also allow measurement of the SN Ia rate out to z Almost-Equal-To 2, providing a complementary constraint on SN Ia progenitor models.« less

  2. STS-103 MS Clervoy and Nicollier and Commander Brown look over Discovery after landing

    NASA Technical Reports Server (NTRS)

    1999-01-01

    After landing at the Shuttle Landing Facility, STS-103 Mission Specialists Jean-Francois Clervoy of France and Claude Nicollier of Switzerland, who are with the European Space Agency, listen to a comment by Commander Curtis L. Brown Jr. while looking over the orbiter Discovery. Other members of the crew are Pilot Scott J. Kelly and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), and John M. Grunsfeld (Ph.D.). The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 EST and wheel stop at 7:01:34 EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history.

  3. KSC-99pp1506

    NASA Image and Video Library

    1999-12-27

    After landing at the Shuttle Landing Facility, the STS-103 crew looks over the orbiter Discovery. In the foreground, from left, are Mission Specialist Jean-Francois Clervoy of France, Pilot Scott J. Kelly, Commander Curtis L. Brown Jr. and Mission Specialist C. Michael Foale (Ph.D.); behind them, from left, are Mission Specialists Steven L. Smith and Claude Nicollier of Switzerland. The remaining crew member (not shown) is Mission Specialist John M. Grunsfeld (Ph.D.). The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  4. KSC-99pp1507

    NASA Image and Video Library

    1999-12-27

    After landing at the Shuttle Landing Facility, STS-103 Mission Specialists Jean-Francois Clervoy of France and Claude Nicollier of Switzerland, who are with the European Space Agency, listen to a comment by Commander Curtis L. Brown Jr. while looking over the orbiter Discovery. Other members of the crew are Pilot Scott J. Kelly and Mission Specialists Steven L. Smith, C. Michael Foale (Ph.D.), and John M. Grunsfeld (Ph.D.). The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  5. Pixel Stability in the Hubble Space Telescope WFC3/UVIS Detector

    NASA Astrophysics Data System (ADS)

    Bourque, Matthew; Baggett, Sylvia M.; Borncamp, David; Desjardins, Tyler D.; Grogin, Norman A.; Wide Field Camera 3 Team

    2018-06-01

    The Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) Ultraviolet-Visible (UVIS) detector has acquired roughly 12,000 dark images since the installation of WFC3 in 2009, as part of a daily monitoring program to measure the instrinsic dark current of the detector. These images have been reconfigured into 'pixel history' images in which detector columns are extracted from each dark and placed into a new time-ordered array, allowing for efficient analysis of a given pixel's behavior over time. We discuss how we measure each pixel's stability, as well as plans for a new Data Quality (DQ) flag to be introduced in a future release of the WFC3 calibration pipeline (CALWF3) for flagging pixels that are deemed unstable.

  6. Hubble Space Telescope

    NASA Image and Video Library

    2017-12-08

    The Hubble Space Telescope in a picture snapped by a Servicing Mission 4 crewmember just after the Space Shuttle Atlantis captured Hubble with its robotic arm on May 13, 2009, beginning the mission to upgrade and repair the telescope. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html

  7. An Optimal Strategy for Accurate Bulge-to-disk Decomposition of Disk Galaxies

    NASA Astrophysics Data System (ADS)

    Gao, Hua; Ho, Luis C.

    2017-08-01

    The development of two-dimensional (2D) bulge-to-disk decomposition techniques has shown their advantages over traditional one-dimensional (1D) techniques, especially for galaxies with non-axisymmetric features. However, the full potential of 2D techniques has yet to be fully exploited. Secondary morphological features in nearby disk galaxies, such as bars, lenses, rings, disk breaks, and spiral arms, are seldom accounted for in 2D image decompositions, even though some image-fitting codes, such as GALFIT, are capable of handling them. We present detailed, 2D multi-model and multi-component decomposition of high-quality R-band images of a representative sample of nearby disk galaxies selected from the Carnegie-Irvine Galaxy Survey, using the latest version of GALFIT. The sample consists of five barred and five unbarred galaxies, spanning Hubble types from S0 to Sc. Traditional 1D decomposition is also presented for comparison. In detailed case studies of the 10 galaxies, we successfully model the secondary morphological features. Through a comparison of best-fit parameters obtained from different input surface brightness models, we identify morphological features that significantly impact bulge measurements. We show that nuclear and inner lenses/rings and disk breaks must be properly taken into account to obtain accurate bulge parameters, whereas outer lenses/rings and spiral arms have a negligible effect. We provide an optimal strategy to measure bulge parameters of typical disk galaxies, as well as prescriptions to estimate realistic uncertainties of them, which will benefit subsequent decomposition of a larger galaxy sample.

  8. An Optimal Strategy for Accurate Bulge-to-disk Decomposition of Disk Galaxies

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gao Hua; Ho, Luis C.

    The development of two-dimensional (2D) bulge-to-disk decomposition techniques has shown their advantages over traditional one-dimensional (1D) techniques, especially for galaxies with non-axisymmetric features. However, the full potential of 2D techniques has yet to be fully exploited. Secondary morphological features in nearby disk galaxies, such as bars, lenses, rings, disk breaks, and spiral arms, are seldom accounted for in 2D image decompositions, even though some image-fitting codes, such as GALFIT, are capable of handling them. We present detailed, 2D multi-model and multi-component decomposition of high-quality R -band images of a representative sample of nearby disk galaxies selected from the Carnegie-Irvine Galaxymore » Survey, using the latest version of GALFIT. The sample consists of five barred and five unbarred galaxies, spanning Hubble types from S0 to Sc. Traditional 1D decomposition is also presented for comparison. In detailed case studies of the 10 galaxies, we successfully model the secondary morphological features. Through a comparison of best-fit parameters obtained from different input surface brightness models, we identify morphological features that significantly impact bulge measurements. We show that nuclear and inner lenses/rings and disk breaks must be properly taken into account to obtain accurate bulge parameters, whereas outer lenses/rings and spiral arms have a negligible effect. We provide an optimal strategy to measure bulge parameters of typical disk galaxies, as well as prescriptions to estimate realistic uncertainties of them, which will benefit subsequent decomposition of a larger galaxy sample.« less

  9. Educational outreach at the NSF Engineering Research Center for Data Storage Systems

    NASA Astrophysics Data System (ADS)

    Williams, James E., Jr.

    1996-07-01

    An aspect of the National Science Foundation Engineering Research Center in Data Storage Systems (DSSC) program that is valued by our sponsors is the way we use our different educational programs to impact the data storage industry in a positive fashion. The most common way to teach data storage materials is in classes that are offered as part of the Carnegie Mellon curriculum. Another way the DSSC attempts to educate students is through outreach programs such as the NSF Research Experiences for Undergraduates and Young Scholars programs, both of which have been very successful and place emphasis and including women, under represented minorities and disable d students. The Center has also established cooperative outreach partnerships which serve to both educate students and benefit the industry. One example is the cooperative program we have had with the Magnetics Technology Centre at the National University of Singapore to help strengthen their research and educational efforts to benefit U.S. data storage companies with plants in Singapore. In addition, the Center has started a program that will help train outstanding students from technical institutes to increase their value as technicians to the data storage industry when they graduate.

  10. Increased structure and active learning reduce the achievement gap in introductory biology.

    PubMed

    Haak, David C; HilleRisLambers, Janneke; Pitre, Emile; Freeman, Scott

    2011-06-03

    Science, technology, engineering, and mathematics instructors have been charged with improving the performance and retention of students from diverse backgrounds. To date, programs that close the achievement gap between students from disadvantaged versus nondisadvantaged educational backgrounds have required extensive extramural funding. We show that a highly structured course design, based on daily and weekly practice with problem-solving, data analysis, and other higher-order cognitive skills, improved the performance of all students in a college-level introductory biology class and reduced the achievement gap between disadvantaged and nondisadvantaged students--without increased expenditures. These results support the Carnegie Hall hypothesis: Intensive practice, via active-learning exercises, has a disproportionate benefit for capable but poorly prepared students.

  11. Hubble’s 25th Anniversary: A Quarter-Century of Discovery and Inspiration

    NASA Astrophysics Data System (ADS)

    Straughn, Amber; Jirdeh, Hussein

    2015-01-01

    April 24, 2015 marks the 25th anniversary of the launch of the Hubble Space Telescope. In its quarter-century in orbit, the Hubble Space Telescope has transformed the way we understand the Universe, helped us find our place among the stars, and paved the way to incredible advancements in science and technology. NASA and ESA, including STScI and partners, will use the 25th anniversary of Hubble's launch as a unique opportunity to communicate to the widest possible audience the significance of the past quarter-century of discovery with the Hubble Space Telescope and to highlight that Hubble will continue to produce groundbreaking science results. We will enhance public understanding of Hubble's many contributions to the scientific world, and will capitalize on Hubble's cultural popularity by emphasizing its' successor, the James Webb Space Telescope. This poster highlights many of the upcoming opportunities to join in the anniversary activities, both in-person and online. Find out more at hubble25th.org and follow #Hubble25 on social media.

  12. A History of the Andrew File System

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Bashear, Derrick

    2011-02-22

    Derrick Brashear and Jeffrey Altman will present a technical history of the evolution of Andrew File System starting with the early days of the Andrew Project at Carnegie Mellon through the commercialization by Transarc Corporation and IBM and a decade of OpenAFS. The talk will be technical with a focus on the various decisions and implementation trade-offs that were made over the course of AFS versions 1 through 4, the development of the Distributed Computing Environment Distributed File System (DCE DFS), and the course of the OpenAFS development community. The speakers will also discuss the various AFS branches developed atmore » the University of Michigan, Massachusetts Institute of Technology and Carnegie Mellon University.« less

  13. Modeling man: the monkey colony at the Carnegie Institution of Washington's Department of Embryology, 1925-1971.

    PubMed

    Wilson, Emily K

    2012-01-01

    Though better recognized for its immediate endeavors in human embryo research, the Carnegie Department of Embryology also employed a breeding colony of rhesus macaques for the purposes of studying human reproduction. This essay follows the course of the first enterprise in maintaining a primate colony for laboratory research and the overlapping scientific, social, and political circumstances that tolerated and cultivated the colony's continued operation from 1925 until 1971. Despite a new-found priority for reproductive sciences in the United States, by the early 1920s an unfertilized human ovum had not yet been seen and even the timing of ovulation remained unresolved. Progress would require an organized research approach that could extend beyond the limitations of working with scant and inherently restrictive human subjects or with common lab mammals like mice. In response, the Department of Embryology, under the Carnegie Institution of Washington (CIW), instituted a novel methodology using a particular primate species as a surrogate in studying normal human reproductive physiology. Over more than 40 years the monkey colony followed an unpremeditated trajectory that would contribute fundamentally to discoveries in human reproduction, early embryo development, reliable birth control methods, and to the establishment of the rhesus macaque as a common model organism.

  14. New Understanding of Hubble Space Telescope Gyro Current Increase Led to a Method to Save a Failing Gyro

    NASA Technical Reports Server (NTRS)

    Blumenstock, Kenneth A.

    2017-01-01

    Throughout the history of the Hubble Space Telescope (HST) program, gyro current increases have been observed to occur, oftentimes leading to gyro failure. The explanation was that debris from the surfaces of the gas bearings, with only 50 millionths on an inch clearance, resulted in rotor restriction, which increased friction, torque, and current. However, the rotor restriction theory never could account for the fact that a restart of the gyro would restore the current back to nominal. An effort was made to understand this puzzling gyro behavior after two HST gyros exhibited increased current within the same week in November 2015. A review board was created to resolve these anomalies and generate operational procedures to potentially extend gyro life.

  15. Low Frequency Flats for Imaging Cameras on the Hubble Space Telescope

    NASA Astrophysics Data System (ADS)

    Kossakowski, Diana; Avila, Roberto J.; Borncamp, David; Grogin, Norman A.

    2017-01-01

    We created a revamped Low Frequency Flat (L-Flat) algorithm for the Hubble Space Telescope (HST) and all of its imaging cameras. The current program that makes these calibration files does not compile on modern computer systems and it requires translation to Python. We took the opportunity to explore various methods that reduce the scatter of photometric observations using chi-squared optimizers along with Markov Chain Monte Carlo (MCMC). We created simulations to validate the algorithms and then worked with the UV photometry of the globular cluster NGC6681 to update the calibration files for the Advanced Camera for Surveys (ACS) and Solar Blind Channel (SBC). The new software was made for general usage and therefore can be applied to any of the current imaging cameras on HST.

  16. What lensed galaxies say about winds and physical conditions in high-z galaxies

    NASA Astrophysics Data System (ADS)

    Rigby, Jane; Gladders, Michael; Sharon, Keren; Wuyts, Eva; Bayliss, Matthew B.; Bordoloi, Rongmon

    2015-08-01

    Gravitational lensing can magnify galaxies by factors of 10--100 times, transforming them from objects we can barely detect to bright objects we can study in detail. I'll summarize new results from a comprehensive program, using imaging from Hubble and Spitzer, and high-quality spectroscopy from Keck, Magellan, and Hubble, to study how galaxies formed stars at redshifts of 1--3, the epoch when most of the Universe's stars were formed. In particularly favorable cases, the imaging and spectra measure variations in physical and wind properties over spatial scales down to ~200 pc. My talk will include results from Bayliss et al. 2014, Wuyts et al. 2014, Whitaker et al. 2014, and Rigby et al. 2014, as well as results not yet published.

  17. Enhancing orbital servicing operations: Providing positive and effective management of spare and installed hardware - A case study of the Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    Randolph, Joseph L.; Shepard, Kenneth E.

    1990-01-01

    The Satellite Resources Management and Tracking System was developed specifically for the Hubble Space Telescope (HST) program, and now, NASA has the ability to immediately access the necessary data for planning successful orbital satellite servicing operations. This system is an online, real-time data base system that contains a plethora of data on each item identified to support the HST throughout its planned 15 year life. Some of the information provided includes the current status, location, quantity, and history of each asset, a separate record for each discrete serial numbered item, procurement lead times on items sensitive to technology obsolescence, and the maintenance and repair history of each asset. Finally, details are provided on organizational, operational and logistics requirements.

  18. Space Shuttle Projects

    NASA Image and Video Library

    2002-03-05

    STS-109 Astronauts Michael J. Massimino and James H. Newman were making their second extravehicular activity (EVA) of their mission when astronaut Massimino, mission specialist, peered into Columbia's crew cabin during a brief break from work on the Hubble Space Telescope (HST). The HST is latched down just a few feet behind him in Columbia's cargo bay. The Space Shuttle Columbia STS-109 mission lifted off March 1, 2002 with goals of repairing and upgrading the Hubble Space Telescope (HST). STS-109 upgrades to the HST included: replacement of the solar array panels; replacement of the power control unit (PCU); replacement of the Faint Object Camera (FOC) with a new advanced camera for Surveys (ACS); and installation of the experimental cooling system for the Hubble's Near-Infrared Camera and Multi-object Spectrometer (NICMOS), which had been dormant since January 1999 when its original coolant ran out. The Marshall Space Flight Center in Huntsville, Alabama had the responsibility for the design, development, and construction of the HST, which is the most powerful and sophisticated telescope ever built. Lasting 10 days, 22 hours, and 11 minutes, the STS-109 mission was the 108th flight overall in NASA's Space Shuttle Program.

  19. STS-109 Astronaut Michael J. Massimino Peers Into Window of Shuttle During EVA

    NASA Technical Reports Server (NTRS)

    2002-01-01

    STS-109 Astronauts Michael J. Massimino and James H. Newman were making their second extravehicular activity (EVA) of their mission when astronaut Massimino, mission specialist, peered into Columbia's crew cabin during a brief break from work on the Hubble Space Telescope (HST). The HST is latched down just a few feet behind him in Columbia's cargo bay. The Space Shuttle Columbia STS-109 mission lifted off March 1, 2002 with goals of repairing and upgrading the Hubble Space Telescope (HST). STS-109 upgrades to the HST included: replacement of the solar array panels; replacement of the power control unit (PCU); replacement of the Faint Object Camera (FOC) with a new advanced camera for Surveys (ACS); and installation of the experimental cooling system for the Hubble's Near-Infrared Camera and Multi-object Spectrometer (NICMOS), which had been dormant since January 1999 when its original coolant ran out. The Marshall Space Flight Center in Huntsville, Alabama had the responsibility for the design, development, and construction of the HST, which is the most powerful and sophisticated telescope ever built. Lasting 10 days, 22 hours, and 11 minutes, the STS-109 mission was the 108th flight overall in NASA's Space Shuttle Program.

  20. The Hubble Deep UV Legacy Survey (HDUV): Survey Overview and First Results

    NASA Astrophysics Data System (ADS)

    Oesch, Pascal; Montes, Mireia; HDUV Survey Team

    2015-08-01

    Deep HST imaging has shown that the overall star formation density and UV light density at z>3 is dominated by faint, blue galaxies. Remarkably, very little is known about the equivalent galaxy population at lower redshifts. Understanding how these galaxies evolve across the epoch of peak cosmic star-formation is key to a complete picture of galaxy evolution. Here, we present a new HST WFC3/UVIS program, the Hubble Deep UV (HDUV) legacy survey. The HDUV is a 132 orbit program to obtain deep imaging in two filters (F275W and F336W) over the two CANDELS Deep fields. We will cover ~100 arcmin2, reaching down to 27.5-28.0 mag at 5 sigma. By directly sampling the rest-frame far-UV at z>~0.5, this will provide a unique legacy dataset with exquisite HST multi-wavelength imaging as well as ancillary HST grism NIR spectroscopy for a detailed study of faint, star-forming galaxies at z~0.5-2. The HDUV will enable a wealth of research by the community, which includes tracing the evolution of the FUV luminosity function over the peak of the star formation rate density from z~3 down to z~0.5, measuring the physical properties of sub-L* galaxies, and characterizing resolved stellar populations to decipher the build-up of the Hubble sequence from sub-galactic clumps. This poster provides an overview of the HDUV survey and presents the reduced data products and catalogs which will be released to the community.

  1. Hubble 25

    NASA Image and Video Library

    2015-04-23

    If you love Hubble as much as we do you will LOVE this video. Sit back and enjoy 25 mesmerizing years of Hubble images! #Hubble25 You can view all of these images on Flickr here: www.flickr.com/photos/40523828@N07/sets/72157649692430461 Credit NASA Goddard

  2. HUBBLE SPIES A REALLY COOL STAR

    NASA Technical Reports Server (NTRS)

    2002-01-01

    This is a Hubble Space Telescope picture of one of the least massive and coolest stars even seen (upper right). It is a diminutive companion to the K dwarf star called GL 105A (also known as HD 16160) seen at lower left. The binary pair is located 27 light-years away in the constellation Cetus. Based on the Hubble observation, astronomers calculate that the companion, called GL 105C, is 25,000 times fainter than GL 105A in visible light. If the dim companion were at the distance of our Sun, it would be only four times brighter than the full moon. The Hubble observations confirm the detection of GL 105C last year by David Golimowski and his collaborators at Palomar Observatory in California. Although GL 105C was identified before, the Hubble view allows a more precise measurement of the separation between the binary components. Future Hubble observations of the binary orbit will allow the masses of both stars to be determined accurately. The Palomar group estimates that the companion's mass is 8-9 percent of the Sun's mass, which places it near the theoretical lower limit for stable hydrogen burning. Objects below this limit, called brown dwarfs, still 'shine' -- not by thermonuclear energy, but by the energy released through gravitational contraction. Two pictures, taken with Hubble's Wide Field Planetary Camera 2 (in PC mode) through different filters (in visible and near-infrared light) show that GL 105C is redder, hence cooler than GL 105A. The surface temperature of GL 105C is not precisely known, but may be as low as 2,600 degrees Kelvin (4,200 degrees Fahrenheit). This image was taken in near-infrared light, on January 5, 1995. GL 105C is located 3.4 arc seconds to the west-northwest of the larger GL 105A. (One arc second equals 1/3600 of a degree.) The bright spikes are caused by diffraction of light within the telescope's optical system, and the brighter white bar is an artifact of the CCD camera, which bleeds along a CCD column when a relatively bright object is in the field of view. These observations are part of a Guaranteed Time Observing Program for which William Fastie (the Johns Hopkins University, Baltimore, MD) and Dan Schroeder (Beloit College, Beloit, WI) were co-principal investigators. Credit: D. Golimowski (Johns Hopkins University), and NASA Image files in GIF and JPEG format may be accessed on Internet via anonymous ftp from oposite.stsci.edu in /pubinfo:

  3. A survey of planning and scheduling research at the NASA Ames Research Center

    NASA Technical Reports Server (NTRS)

    Zweben, Monte

    1989-01-01

    NASA Ames Research Center has a diverse program in planning and scheduling. Some research projects as well as some applications are highlighted. Topics addressed include machine learning techniques, action representations and constraint-based scheduling systems. The applications discussed are planetary rovers, Hubble Space Telescope scheduling, and Pioneer Venus orbit scheduling.

  4. Three Axis Control of the Hubble Space Telescope Using Two Reaction Wheels and Magnetic Torquer Bars for Science Observations

    NASA Technical Reports Server (NTRS)

    Hur-Diaz, Sun; Wirzburger, John; Smith, Dan

    2008-01-01

    The Hubble Space Telescope (HST) is renowned for its superb pointing accuracy of less than 10 milli-arcseconds absolute pointing error. To accomplish this, the HST relies on its complement of four reaction wheel assemblies (RWAs) for attitude control and four magnetic torquer bars (MTBs) for momentum management. As with most satellites with reaction wheel control, the fourth RWA provides for fault tolerance to maintain three-axis pointing capability should a failure occur and a wheel is lost from operations. If an additional failure is encountered, the ability to maintain three-axis pointing is jeopardized. In order to prepare for this potential situation, HST Pointing Control Subsystem (PCS) Team developed a Two Reaction Wheel Science (TRS) control mode. This mode utilizes two RWAs and four magnetic torquer bars to achieve three-axis stabilization and pointing accuracy necessary for a continued science observing program. This paper presents the design of the TRS mode and operational considerations necessary to protect the spacecraft while allowing for a substantial science program.

  5. hs-2007-16-e-full_jpg

    NASA Image and Video Library

    2010-03-01

    Carina Nebula Details: The Caterpillar Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA) Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html

  6. Hubble Against Earth Horizon 1997

    NASA Image and Video Library

    1997-10-10

    The Hubble Space Telescope hovers at the boundary of Earth and space in this picture, taken after Hubble second servicing mission in 1997. Hubble drifts 353 miles (569 km) above the Earth's surface, where it can avoid the atmosphere and clearly see objects in space. http://photojournal.jpl.nasa.gov/catalog/PIA18165

  7. Stability of the Zagreb realization of the Carnegie-Mellon-Berkeley coupled-channels unitary model

    NASA Astrophysics Data System (ADS)

    Osmanović, H.; Ceci, S.; Švarc, A.; Hadžimehmedović, M.; Stahov, J.

    2011-09-01

    In Hadžimehmedović [Phys. Rev. CPRVCAN0556-281310.1103/PhysRevC.84.035204 84, 035204 (2011)] we have used the Zagreb realization of Carnegie-Melon-Berkeley coupled-channel, unitary model as a tool for extracting pole positions from the world collection of partial-wave data, with the aim of eliminating model dependence in pole-search procedures. In order that the method is sensible, we in this paper discuss the stability of the method with respect to the strong variation of different model ingredients. We show that the Zagreb CMB procedure is very stable with strong variation of the model assumptions and that it can reliably predict the pole positions of the fitted partial-wave amplitudes.

  8. Barred Spiral Galaxy

    NASA Image and Video Library

    2017-12-08

    Barred Spiral Galaxy NGC 1300 Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA) Acknowledgment: P. Knezek (WIYN) The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html

  9. RR Lyrae period luminosity relations with Spitzer

    NASA Astrophysics Data System (ADS)

    Neeley, Jillian R.; Marengo, Massimo; CRRP Team

    2017-01-01

    RR Lyrae variable stars have long been known to be valuable distance indicators, but only recently has a well defined period luminosity relationship been utilized at infrared wavelengths. In my thesis, I am combining Spitzer Space Telescope data of RR Lyrae stars obtained as part of the Carnegie RR Lyrae Program with ground based NIR data to characterize the period-luminosity-metallicity (PLZ) relation and provide an independent Population II calibration of the cosmic distance scale. I will discuss the ongoing efforts to calibrate this relation using objects such as M4 and NGC 6441 and how the first data release from the Gaia mission impacts our findings. I will also compare my preliminary empirical relations to theoretical PLZ relations derived from stellar pulsation models.

  10. KSC-02pd0097

    NASA Image and Video Library

    2002-01-29

    KENNEDY SPACE CENTER, FLA. - Workers in the Vertical Processing Facility check the position of the Hubble Space Telescope's replacement Reaction Wheel Actuator on the Large Orbital Protective Enclosure (LOPE), which is contained in the Multi-Use Lightweight Equipment (MULE) for flight. Part of Hubble's Pointing Control System, the actuators receiving information from sensors and physically adjust Hubble's position and orientation so that Hubble can view the required celestial bodies. The reaction wheels work by rotating a large flywheel up to 3000 rpm or braking it to exchange momentum with the spacecraft which will make Hubble turn. The RWA is part of the payload on mission STS-109, the Hubble Servicing Mission, scheduled to launch Feb. 28, 2002

  11. KSC-02pd0095

    NASA Image and Video Library

    2002-01-29

    KENNEDY SPACE CENTER, FLA. - Workers in the Vertical Processing Facility maneuver the replacement Reaction Wheel Actuator for the Hubble Space Telescope into position on the Large Orbital Protective Enclosure (LOPE), which is contained in the Multi-Use Lightweight Equipment (MULE) for flight. Part of Hubble's Pointing Control System, the actuators receiving information from sensors and physically adjust Hubble's position and orientation so that Hubble can view the required celestial bodies. The reaction wheels work by rotating a large flywheel up to 3000 rpm or braking it to exchange momentum with the spacecraft which will make Hubble turn. The RWA is part of the payload on mission STS-109, the Hubble Servicing Mission, scheduled to launch Feb. 28, 2002

  12. KSC-02pd0098

    NASA Image and Video Library

    2002-01-29

    KENNEDY SPACE CENTER, FLA. -- Workers in the Vertical Processing Facility check the attachment of the the Hubble Space Telescope's replacement Reaction Wheel Actuator on the Large Orbital Protective Enclosure (LOPE), which is contained in the Multi-Use Lightweight Equipment (MULE) for flight. Part of Hubble's Pointing Control System, the actuators receiving information from sensors and physically adjust Hubble's position and orientation so that Hubble can view the required celestial bodies. The reaction wheels work by rotating a large flywheel up to 3000 rpm or braking it to exchange momentum with the spacecraft which will make Hubble turn. The RWA is part of the payload on mission STS-109, the Hubble Servicing Mission, scheduled to launch Feb. 28, 2002

  13. The Hubble Frontier Fields: Engaging Multiple Audiences in Exploring the Cosmic Frontier

    NASA Astrophysics Data System (ADS)

    Lawton, Brandon L.; Smith, Denise A.; Summers, Frank; Ryer, Holly; Slivinski, Carolyn; Lotz, Jennifer M.

    2017-06-01

    The Hubble Frontier Fields is a multi-cycle program of six deep-field observations of strong-lensing galaxy clusters taken in parallel with six deep “blank fields.” The three-year long collaborative program began in late 2013 and is led by observations from NASA’s Great Observatories. The observations, now complete, allow astronomers to look deeper into the universe than ever before, and potentially uncover galaxies that are as much as 100 times fainter than what the telescopes can typically observe. The Frontier Fields science program is ideal for informing audiences about scientific advances and topics in STEM. The study of galaxy properties, statistics, optics, and Einstein’s theory of general relativity naturally leverages off of the science returns of the Frontier Fields program. As a result, the Space Telescope Science Institute’s Office of Public Outreach (OPO) has engaged multiple audiences over the past three years to follow the progress of the Frontier Fields.For over two decades, the STScI outreach program has sought to bring the wonders of the universe to the public and engage audiences in the adventure of scientific discovery. In addition, we are leveraging the reach of the new NASA’s Universe of Learning education program to bring the science of the Frontier Fields to informal education audiences. The main underpinnings of the STScI outreach program and the Universe of Learning education program are scientist-educator development teams, partnerships, and an embedded program evaluation component. OPO is leveraging the infrastructure of these education and outreach programs to bring the Frontier Fields science program to the education community and the public in a cost-effective way.This talk will feature highlights over the past three years of the program. We will highlight OPO’s strategies and infrastructure that allows for the quick delivery of groundbreaking science to the education community and public.

  14. HST PSF simulation using Tiny Tim

    NASA Technical Reports Server (NTRS)

    Krist, J. E.

    1992-01-01

    Tiny Tim is a program which simulates Hubble Space Telescope imaging camera PSF's. It is portable (written and distributed in C) and is reasonably fast. It can model the WFPC, WFPC 2, FOC, and COSTAR corrected FOC cameras. In addition to aberrations such as defocus and spherical, it also includes WFPC obscuration shifting, mirror zonal error maps, and jitter. The program has been used at a number of sites for deconvolving HST images. Tiny Tim is available via anonymous ftp on stsci.edu in the directory software/tinytim.

  15. Causes of catastrophic failure in complex systems

    NASA Astrophysics Data System (ADS)

    Thomas, David A.

    2010-08-01

    Root causes of mission critical failures and major cost and schedule overruns in complex systems and programs are studied through the post-mortem analyses compiled for several examples, including the Hubble Space Telescope, the Challenger and Columbia Shuttle accidents, and the Three Mile Island nuclear power plant accident. The roles of organizational complexity, cognitive biases in decision making, the display of quantitative data, and cost and schedule pressure are all considered. Recommendations for mitigating the risk of similar failures in future programs are also provided.

  16. Policy opportunities

    NASA Technical Reports Server (NTRS)

    Mccray, Richard; Ostriker, Jeremiah P.; Acton, Loren W.; Bahcall, Neta A.; Bless, Robert C.; Brown, Robert A.; Burbidge, Geoffrey; Burke, Bernard F.; Clark, George W.; Cordova, France A.

    1991-01-01

    Recommendations are given regarding National Science Foundation (NSF) astronomy programs and the NASA Space Astrophysics program. The role of ground based astronomy is reviewed. The role of National Optical Astronomy Observatories (NOAO) in ground-based night-time astronomical research is discussed. An enhanced Explored Program, costs and management of small and moderate space programs, the role of astrophysics within NASA's space exploration initiative, suborbital and airborne astronomical research, the problems of the Hubble Space Telescope, and astronomy education are discussed. Also covered are policy issues related to the role of science advisory committees, international cooperation and competition, archiving and distribution of astronomical data, and multi-wavelength observations of variable sources.

  17. Laryngeal findings and acoustic changes in hubble-bubble smokers.

    PubMed

    Hamdan, Abdul-latif; Sibai, Abla; Oubari, Dima; Ashkar, Jihad; Fuleihan, Nabil

    2010-10-01

    The purpose of our investigation was to evaluate the laryngeal findings and acoustic changes in hubble-bubble smokers. A total of 42 subjects with history of hubble-bubble smoking were recruited for this study. A corresponding group with a history of cigarette smoking and controls were matched. All subjects underwent laryngeal video-endostroboscopic evaluation and acoustic analysis. In the hubble-bubble smoking group, 61.9% were males. The average age was 30.02 +/- 9.48 years and the average number of years of smoking was 8.09 +/- 6.45 years. Three subjects had dysphonia at the time of examination. The incidence of benign lesions of the vocal folds in the hubble-bubble group was 21.5%, with edema being the most common at 16.7% followed by cyst at 4.8%. The incidence of laryngeal findings was significantly higher in the hubble-bubble group compared to controls. In the cigarette-smoking group, the most common finding was vocal fold cyst in 14.8% followed by polyps in 7.4%, and edema, sulcus vocalis and granuloma. These findings were not significantly different from the hubble-bubble group except for the thick mucus, which was significantly higher in the latter. There were no significant changes in any of the acoustic parameters between hubble-bubble smokers and controls except for the VTI and MPT, which were significantly lower in the hubble-bubble group. In comparison with the cigarette-smoking group, hubble-bubble smokers had significantly higher Fundamental frequency and habitual pitch (p value 0.042 and 0.008, respectively). The laryngeal findings in hubble-bubble smokers are comparable to cigarette smokers. These laryngeal findings are not translated acoustically, as all the acoustic parameters are within normal range compared to controls.

  18. NASA’s Hubble Telescope Finds Potential Kuiper Belt Targets for New Horizons Pluto Mission

    NASA Image and Video Library

    2017-12-08

    This is an artist’s impression of a Kuiper Belt object (KBO), located on the outer rim of our solar system at a staggering distance of 4 billion miles from the Sun. A HST survey uncovered three KBOs that are potentially reachable by NASA’s New Horizons spacecraft after it passes by Pluto in mid-2015. Credit: NASA, ESA, and G. Bacon (STScI) --- Peering out to the dim, outer reaches of our solar system, NASA’s Hubble Space Telescope has uncovered three Kuiper Belt objects (KBOs) the agency’s New Horizons spacecraft could potentially visit after it flies by Pluto in July 2015. The KBOs were detected through a dedicated Hubble observing program by a New Horizons search team that was awarded telescope time for this purpose. “This has been a very challenging search and it’s great that in the end Hubble could accomplish a detection – one NASA mission helping another,” said Alan Stern of the Southwest Research Institute (SwRI) in Boulder, Colorado, principal investigator of the New Horizons mission. The Kuiper Belt is a vast rim of primordial debris encircling our solar system. KBOs belong to a unique class of solar system objects that has never been visited by spacecraft and which contain clues to the origin of our solar system. The KBOs Hubble found are each about 10 times larger than typical comets, but only about 1-2 percent of the size of Pluto. Unlike asteroids, KBOs have not been heated by the sun and are thought to represent a pristine, well preserved deep-freeze sample of what the outer solar system was like following its birth 4.6 billion years ago. The KBOs found in the Hubble data are thought to be the building blocks of dwarf planets such as Pluto. Read more: 1.usa.gov/1vzUcyK NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram

  19. Micrometeoroid Impacts on the Hubble Sace Telescope Wide Field and Planetary Camera 2: Ion Beam Analysis of Subtle Impactor Traces

    NASA Technical Reports Server (NTRS)

    Grime, G. W.; Webb, R. P.; Jeynes, C.; Palitsin, V. V.; Colaux, J. L.; Kearsley, A. T.; Ross, D. K.; Anz-Meador, P.; Liou, J. C.; Opiela, J.; hide

    2014-01-01

    Recognition of origin for particles responsible for impact damage on spacecraft such as the Hubble Space Telescope (HST) relies upon postflight analysis of returned materials. A unique opportunity arose in 2009 with collection of the Wide Field and Planetary Camera 2 (WFPC2) from HST by shuttle mission STS-125. A preliminary optical survey confirmed that there were hundreds of impact features on the radiator surface. Following extensive discussion between NASA, ESA, NHM and IBC, a collaborative research program was initiated, employing scanning electron microscopy (SEM) and ion beam analysis (IBA) to determine the nature of the impacting grains. Even though some WFPC2 impact features are large, and easily seen without the use of a microscope, impactor remnants may be hard to find.

  20. Maintaining an expert system for the Hubble Space Telescope ground support

    NASA Technical Reports Server (NTRS)

    Lindenmayer, Kelly; Vick, Shon; Rosenthal, Don

    1987-01-01

    The transformation portion of the Hubble Space Telescope (HST) Proposal Entry Processor System converts astronomer-oriented description of a scientific observing program into a detailed description of the parameters needed for planning and scheduling. The transformation system is one of a very few rulebased expert systems that has ever entered an operational phase. The day to day operations of the system and its rulebase are no longer the responsibility of the original developer. As a result, software engineering properties of the rulebased approach become more important. Maintenance issues associated with the coupling of rules within a rulebased system are discussed and a method is offered for partitioning a rulebase so that the amount of knowledge needed to modify the rulebase is minimized. This method is also used to develop a measure of the coupling strength of the rulebase.

  1. Fabrication of MgF2 and LiF windows for the Hubble Space Telescope Imaging Spectrograph

    NASA Technical Reports Server (NTRS)

    Gormley, Daphne; Bottema, Murk; Darnell, Barbara; Fowler, Walter; Medenica, Walter

    1988-01-01

    Two prototype test windows (MgF2 and LiF) to be used on the 75-mm UV MAMA detector tubes for the Hubble Space Telescope Imaging Spectrograph are described. The spatial and optical constraints of this instrument dictate that the thickness of the window materials be no greater than 2-3 mm to achieve a minimum 50-percent transmission at hydrogen Lyman alpha (121.6 nm), and that the window must be domed to minimize optical aberrations and provide structural strength. The detector window has an input diameter of about 100 mm with a radius-of-curvature of 70 mm. The manufacturing processes involved in the fabrication of these windows is discussed, as well as test programs (optical and structural) to be performed at Goddard Space Flight Center.

  2. Hubble Space Telescope cycle 5 call for proposals

    NASA Technical Reports Server (NTRS)

    Bond, Howard E. (Editor)

    1994-01-01

    This document invites and supports participation by the international astronomical community in the HST General Observer and Archival Research programs. These documents contain the basic procedural and technical information required for HST proposal preparation and submission, including applicable deadlines. The telescope and its instruments were built under the auspices of the NASA and the European Space Agency.

  3. Probing the z > 6 Universe with the First Hubble Frontier Fields Cluster A2744

    NASA Astrophysics Data System (ADS)

    Atek, Hakim; Richard, Johan; Kneib, Jean-Paul; Clement, Benjamin; Egami, Eiichi; Ebeling, Harald; Jauzac, Mathilde; Jullo, Eric; Laporte, Nicolas; Limousin, Marceau; Natarajan, Priyamvada

    2014-05-01

    The Hubble Frontier Fields program combines the capabilities of the Hubble Space Telescope (HST) with the gravitational lensing of massive galaxy clusters to probe the distant universe to an unprecedented depth. Here, we present the results of the first combined HST and Spitzer observations of the cluster A-2744. We combine the full near-infrared data with ancillary optical images to search for gravitationally lensed high-redshift (z >~ 6) galaxies. We report the detection of 15 I 814 dropout candidates at z ~ 6-7 and one Y 105 dropout at z ~ 8 in a total survey area of 1.43 arcmin2 in the source plane. The predictions of our lens model also allow us to identify five multiply imaged systems lying at redshifts between z ~ 6 and z ~ 8. Thanks to constraints from the mass distribution in the cluster, we were able to estimate the effective survey volume corrected for completeness and magnification effects. This was in turn used to estimate the rest-frame ultraviolet luminosity function (LF) at z ~ 6-8. Our LF results are generally in agreement with the most recent blank field estimates, confirming the feasibility of surveys through lensing clusters. Although based on a shallower observations than what will be achieved in the final data set including the full Advanced Camera for Survey observations, the LF presented here goes down to M UV ~-18.5, corresponding to 0.2L sstarf at z ~ 7 with one identified object at M UV ~-15 thanks to the highly magnified survey areas. This early study forecasts the power of using massive galaxy clusters as cosmic telescopes and its complementarity to blank fields. Based on observations made with the NASA/ESA Hubble Space Telescope (HST), which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs 13495 and 11689. Based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work utilizes gravitational lensing models produced by PIs Ebeling, Merten, and Zitrin, and Sharon funded as part of the HST Frontier Fields program conducted by STScI. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. The lens models were obtained from the Mikulski Archive for Space Telescopes (MAST).

  4. RR Lyrae Stars as High-Precision Standard Candles in the Mid-Infrared

    NASA Astrophysics Data System (ADS)

    Neeley, Jillian Rose

    In this work, we provide the theoretical and empirical framework to establish RR Lyrae stars (RRL) as the anchor of a Population II distance scale. We present new theoretical period-luminosity-metallicity (PLZ) relations for RRL at Spitzer and WISE wavelengths. The PLZ relations were derived using nonlinear, time-dependent convective hydrodynamical models for a broad range in metal abundances (Z = 0.0001 to 0.0198). We also compare our theoretical relations to empirical relations derived from RRL in the field. Our theoretical PLZ relations were combined with multi-wavelength observations to simultaneously fit the distance modulus and extinction of each individual Galactic RRL in our sample. The results are consistent with trigonometric parallax measurements from the Gaia mission's first data release. This analysis has shown that when considering a sample covering a typical range of iron abundances for RRL, the metallicity spread introduces a dispersion in the PL relation on the order of 0.13 mag. However, if this metallicity component is accounted for in a PLZ relation, the dispersion is reduced to 0.02 mag at MIR wavelengths. On the empirical side, we present the analysis of five clusters from the Carnegie RR Lyrae Program (CRRP) sample (M4, NGC 3201, M5, M15, and M14). M4, the nearest one of the most well studied clusters, was used as a test case to develop a new data analysis pipeline for CRRP. Following the analysis of the five clusters, the resulting calibration PL relations are M[3.6] = -2.424 +/- 0.079 log P -1.205 +/- 0.057 and M [4.5] = -2.245 +/- 0.076 - 1.225 +/- 0.057. The slope of the PL relations was determined from the weighted average of the cluster results, and the zero point was fixed using five Galactic RRL with geometric parallaxes measured by Hubble Space Telescope. The dispersion of the RRL around the PL relations ranges from 0.05 mag in M4 to 0.3 mag in M14. The resulting band-averaged distance moduli for the five clusters agree well with results in the literature. The systematic uncertainty will be greatly reduced when parallaxes of more stars become available from the Gaia mission, and we are able to use the full CRRP sample of 55 Galactic RRL to calibrate the relation.

  5. Embryonic cardiac morphometry in Carnegie stages 15-23, from the Complutense University of Madrid Institute of Embryology Human Embryo Collection.

    PubMed

    Arráez-Aybar, L A; Turrero-Nogués, A; Marantos-Gamarra, D G

    2008-01-01

    We performed a morphometric study of cardiac development on human embryos to complement the scarce data on human embryonic cardiac morphometry and to attempt to establish, from these, algorithms describing cardiac growth during the second month of gestation. Thirty human embryos from Carnegie stages 15-23 were included in the study. Shrinkage and compression effects from fixation and inclusion in paraffin were considered in our calculations. Growth of the cardiac (whole heart) volume and volume of ventricular myocardium through the Carnegie stages were analysed by ANOVA. Linear correlation was used to describe the relationship between the ventricular myocardium and cardiac volumes. Comparisons of models were carried out through the R2 statistic. The relationship volume of ventricular myocardium versus cardiac volume is expressed by the equation: cardiac volume = 0.6266 + 2.4778 volume of ventricular myocardium. The relationship cardiac volume versus crown-rump length is expressed by the equation: cardiac volume = 1.3 e(0.126 CR length), where e is the base of natural logarithms. At a clinical level, these results can contribute towards the establishment of a normogram for cardiac development, useful for the design of strategies for early diagnosis of congenital heart disease. They can also help in the study of embryogenesis, for example in the discussion of ventricular trabeculation. Copyright 2007 S. Karger AG, Basel.

  6. Carnegie Science Academy Web Site

    NASA Astrophysics Data System (ADS)

    Kotwicki, John; Atzinger, Joe; Turso, Denise

    1997-11-01

    The Carnegie Science Academy is a professional society "For Teens...By Teens" at the Carnegie Science Center in Pittsburgh. The CSA Web Site [ http://csa.clpgh.org ] is designed for teens who have an interest in science and technology. This online or virtual science academy provides resources for teens in high school science classes. The Web site also allows students around the world to participate and communicate with other students, discuss current events in science, share opinions, find answers to questions, or make online friends. Visitors can enjoy the main components of the site or sign up for a free membership which allows access to our chat room for monthly meeting, online newsletter, members forum, and much more. Main components to the site include a spot for cool links and downloads, available for any visitor to download or view. Online exhibits are created by students to examine and publish an area of study and also allow teachers to easily post classroom activities as exhibits by submitting pictures and text. Random Access, the interactive part of the academy, allows users to share ideas and opinions. Planet CSA focuses on current events in science and the academy. In the future the CSA Web site will become a major resource for teens and science teachers providing materials that will allow students to further enhance their interest and experiences in science.

  7. KSC-99pp1508

    NASA Image and Video Library

    1999-12-27

    As he exits the Crew Hatch Access Vehicle, STS-103 Commander Curtis L. Brown Jr. is greeted with a handshake by Joseph Rothenberg, associate administrator, Office of Space Flight. Descending the stairs behind Brown are (left to right) Mission Specialists C. Michael Foale (Ph.D.) and John M. Grunsfeld (Ph.D.) and Pilot Scott J. Kelly. At right, applauding the astronauts return are Earle Huckins, deputy associate administrator, Office of Space Science, and Roy Bridges, director, Kennedy Space Center. Others in the crew (not shown) are Mission Specialists Steven L. Smith, and Jean-Francois Clervoy of France and Claude Nicollier of Switzerland, who are with the European Space Agency. The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 p.m. EST and wheel stop at 7:01:34 p.m. EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history

  8. STS-103 crew is greeted after exiting the Crew Hatch Access Vehicle

    NASA Technical Reports Server (NTRS)

    1999-01-01

    As he exits the Crew Hatch Access Vehicle, STS-103 Commander Curtis L. Brown Jr. is greeted with a handshake by Joseph Rothenberg, associate administrator, Office of Space Flight. Descending the stairs behind Brown are (left to right) Mission Specialists C. Michael Foale (Ph.D.) and John M. Grunsfeld (Ph.D.) and Pilot Scott J. Kelly. At right, applauding the astronauts return are Earle Huckins, deputy associate administrator, Office of Space Science, and Roy Bridges, director, Kennedy Space Center. Others in the crew (not shown) are Mission Specialists Steven L. Smith, and Jean-Francois Clervoy of France and Claude Nicollier of Switzerland, who are with the European Space Agency. The crew of seven completed a successful eight-day mission to service the Hubble Space Telescope, spending the Christmas holiday in space in order to accomplish their mission before the end of 1999. During the mission, Discovery's four space-walking astronauts, Smith, Foale, Grunsfeld and Nicollier, spent 24 hours and 33 minutes upgrading and refurbishing Hubble, making it more capable than ever to renew its observations of the universe. Mission objectives included replacing gyroscopes and an old computer, installing another solid state recorder, and replacing damaged insulation in the telescope. Hubble was released from the end of Discovery's robot arm on Christmas Day. Main gear touchdown was at 7:00:47 p.m. EST. Nose gear touchdown occurred at 7:00:58 EST and wheel stop at 7:01:34 EST. This was the 96th flight in the Space Shuttle program and the 27th for the orbiter Discovery. The landing was the 20th consecutive Shuttle landing in Florida and the 13th night landing in Shuttle program history.

  9. NASA's Hubble Celebrates 21st Anniversary with "Rose" of Galaxies

    NASA Image and Video Library

    2017-12-08

    NASA image release April 20, 2011 To see a video of this image go here: www.flickr.com/photos/gsfc/5637796622 To celebrate the 21st anniversary of the Hubble Space Telescope's deployment into space, astronomers at the Space Telescope Science Institute in Baltimore, Md., pointed Hubble's eye at an especially photogenic pair of interacting galaxies called Arp 273. The larger of the spiral galaxies, known as UGC 1810, has a disk that is distorted into a rose-like shape by the gravitational tidal pull of the companion galaxy below it, known as UGC 1813. This image is a composite of Hubble Wide Field Camera 3 data taken on December 17, 2010, with three separate filters that allow a broad range of wavelengths covering the ultraviolet, blue, and red portions of the spectrum. Hubble was launched April 24, 1990, aboard Discovery's STS-31 mission. Hubble discoveries revolutionized nearly all areas of current astronomical research from planetary science to cosmology. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) To read more about this image go here: www.nasa.gov/mission_pages/hubble/science/hubble-rose.html NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on Facebook

  10. Wings in Orbit: Scientific and Engineering Legacies of the Space Shuttle, 1971-2010

    NASA Technical Reports Server (NTRS)

    Hale, Wayne (Editor); Lane, Helen (Editor); Chapline, Gail (Editor); Lulla, Kamlesh (Editor)

    2011-01-01

    The Space Shuttle is an engineering marvel perhaps only exceeded by the station itself. The shuttle was based on the technology of the 1960s and early 1970s. It had to overcome significant challenges to make it reusable. Perhaps the greatest challenges were the main engines and the Thermal Protection System. The program has seen terrible tragedy in its 3 decades of operation, yet it has also seen marvelous success. One of the most notable successes is the Hubble Space Telescope, a program that would have been a failure without the shuttle's capability to rendezvous, capture, repair, as well as upgrade. Now Hubble is a shining example of success admired by people around the world. As the program comes to a close, it is important to capture the legacy of the shuttle for future generations. That is what "Wings In Orbit" does for space fans, students, engineers, and scientists. This book, written by the men and women who made the program possible, will serve as an excellent reference for building future space vehicles. We are proud to have played a small part in making it happen. Our journey to document the scientific and engineering accomplishments of this magnificent winged vehicle began with an audacious proposal: to capture the passion of those who devoted their energies to its success while answering the question "What are the most significant accomplishments?" of the longestoperating human spaceflight program in our nation s history. This is intended to be an honest, accurate, and easily understandable account of the research and innovation accomplished during the era.

  11. VizieR Online Data Catalog: Galaxy samples rest-frame ultraviolet structure (Bond+, 2014)

    NASA Astrophysics Data System (ADS)

    Bond, N. A.; Gardner, J. P.; de Mello, D. F.; Teplitz, H. I.; Rafelski, M.; Koekemoer, A. M.; Coe, D.; Grogin, N.; Gawiser, E.; Ravindranath, S.; Scarlata, C.

    2017-03-01

    In this paper, we use data taken as part of a program (GO 11563, PI: Teplitz) to obtain UV imaging of the Hubble Ultra Deep Field (hereafter UVUDF) and study intermediate-redshift galaxy structure in the F336W, F275W, and F225W filters, complementing existing optical and near-IR measurements from the 2012 Hubble Ultra Deep Field (HUDF12; Ellis et al. 2013ApJ...763L...7E) survey. We use AB magnitudes throughout and assume a concordance cosmology with H0=71 km/s/Mpc, ωm=0.27, and ωλ=0.73 (Spergel et al. 2007ApJS..170..377S). The UVUDF data and the optical Hubble Ultradeep Field (UDF; Beckwith et al. 2006, J/AJ/132/1729) are both contained within a single deep field in the Great Observatories Origins Deep Survey South. The new UVUDF data include imaging in three filters (F336W, F275W, and F225W), obtained in 10 visits, for a total of 30 orbits per filter. In addition, from the UDF, we make use of deep drizzled images taken in the observed optical with the F435W, F606W, and F775W filters. (1 data file).

  12. Periconceptional maternal one-carbon biomarkers are associated with embryonic development according to the Carnegie stages.

    PubMed

    Parisi, F; Rousian, M; Koning, A H J; Willemsen, S P; Cetin, I; Steegers-Theunissen, R P M

    2017-03-01

    Is periconceptional maternal one-carbon (I-C) metabolism associated with embryonic morphological development in non-malformed ongoing pregnancies? Serum vitamin B12, red blood cell (RBC) folate and plasma total homocysteine (tHcy) are associated with embryonic development according to the Carnegie stages. Derangements in maternal I-C metabolism affect reproductive and pregnancy outcomes, as well as future health of the offspring. Between 2010 and 2014, women with singleton ongoing pregnancies were enrolled in a prospective periconceptional cohort study. A total of 234 pregnancies, including 138 spontaneous or IUI pregnancies with strict pregnancy dating and 96 pregnancies derived from IVF, ICSI or cryopreserved embryo transfer (IVF/ICSI pregnancies), underwent longitudinal transvaginal three-dimensional ultrasound (3D US) scans from 6+0 up to 10+2 weeks of gestation. Carnegie stages were defined using internal and external morphologic criteria in a virtual reality system. Maternal venous blood samples were collected at enrollment for serum vitamin B12, RBC folate and plasma tHcy assessment. Associations between biomarker concentrations and longitudinal Carnegie stages were investigated using linear mixed models. We performed a median of three 3D US scans per pregnancy (range 1-5) resulting in 600 good quality data sets for the Carnegie stage annotation (80.5%). Vitamin B12 was positively associated with embryonic development in the total study population (β = 0.001 (95% CI: 0.000; 0.002), P < 0.05) and in the subgroup of strictly dated spontaneous pregnancies (β = 0.002 (95% CI: 0.001; 0.003), P < 0.05). Low vitamin B12 concentrations (-2SD, 73.4 pmol/l) were associated with delayed embryonic development by 1.4 days (95% CI: 1.3-1.4) compared with high concentrations (+2SD, 563.1 pmol/l). RBC folate was positively associated with Carnegie stages only in IVF/ICSI pregnancies (β = 0.001 (95% CI: 0.0005; 0.0015), P < 0.05). In this group, low RBC folate concentrations (-2SD, 875.4 nmol/l) were associated with a 1.8-day delay (95% CI: 1.7-1.8) in development compared with high concentrations (+2SD, 2119.9 nmol/l). tHcy was negatively associated with embryonic development in the total study population (β = -0.08 (95% CI: -0.14; -0.02), P < 0.01), as well as in the IVF/ICSI subgroup (β = -0.08 (95% CI: -0.15; -0.01), P < 0.05). High tHcy concentrations (+2SD, 10.4 µmol/l) were associated with a delay of 1.6 days (95% CI: 1.5-1.7) in embryonic development compared with low concentrations (-2SD, 3.0 µmol/l). The study was performed in a tertiary care center, resulting in high rates of folic acid supplement use and comorbidity that may reduce the external validity of our findings. In periconceptional care, maternal I-C biomarkers should be taken into account as predictors of embryonic morphological development. Combining embryonic size measurements with morphological assessment could better define normal embryonic development. The work was funded by the Department of Obstetrics and Gynaecology, Erasmus MC, University Medical Centre, Rotterdam, The Netherlands. RPMST is CSO of the startup company Slimmere Zorg and CEO of eHealth Care Solutions. The authors declare no conflicts of interest. Not applicable. © The Author 2017. Published by Oxford University Press on behalf of the European Society of Human Reproduction and Embryology. All rights reserved. For permissions, please e-mail: journals.permissions@oup.com

  13. HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses

    NASA Astrophysics Data System (ADS)

    Shipley, Heath V.; Lange-Vagle, Daniel; Marchesini, Danilo; Brammer, Gabriel B.; Ferrarese, Laura; Stefanon, Mauro; Kado-Fong, Erin; Whitaker, Katherine E.; Oesch, Pascal A.; Feinstein, Adina D.; Labbé, Ivo; Lundgren, Britt; Martis, Nicholas; Muzzin, Adam; Nedkova, Kalina; Skelton, Rosalind; van der Wel, Arjen

    2018-03-01

    We present Hubble multi-wavelength photometric catalogs, including (up to) 17 filters with the Advanced Camera for Surveys and Wide Field Camera 3 from the ultra-violet to near-infrared for the Hubble Frontier Fields and associated parallels. We have constructed homogeneous photometric catalogs for all six clusters and their parallels. To further expand these data catalogs, we have added ultra-deep K S -band imaging at 2.2 μm from the Very Large Telescope HAWK-I and Keck-I MOSFIRE instruments. We also add post-cryogenic Spitzer imaging at 3.6 and 4.5 μm with the Infrared Array Camera (IRAC), as well as archival IRAC 5.8 and 8.0 μm imaging when available. We introduce the public release of the multi-wavelength (0.2–8 μm) photometric catalogs, and we describe the unique steps applied for the construction of these catalogs. Particular emphasis is given to the source detection band, the contamination of light from the bright cluster galaxies (bCGs), and intra-cluster light (ICL). In addition to the photometric catalogs, we provide catalogs of photometric redshifts and stellar population properties. Furthermore, this includes all the images used in the construction of the catalogs, including the combined models of bCGs and ICL, the residual images, segmentation maps, and more. These catalogs are a robust data set of the Hubble Frontier Fields and will be an important aid in designing future surveys, as well as planning follow-up programs with current and future observatories to answer key questions remaining about first light, reionization, the assembly of galaxies, and many more topics, most notably by identifying high-redshift sources to target.

  14. Automated Inspection of Aircraft

    DOT National Transportation Integrated Search

    1998-04-01

    This report summarizes the development of a robotic system designed to assist aircraft inspectors by remotely deploying non-destructive inspection (NDI) sensors and acquiring, processing, and storing inspection data. Carnegie Mellon University studie...

  15. Hubble Captures Detailed Image of Uranus Atmosphere

    NASA Image and Video Library

    1998-08-02

    NASA Hubble Space Telescope peered deep into Uranus atmosphere to see clear and hazy layers created by a mixture of gases. Using infrared filters, Hubble captured detailed features of three layers of Uranus atmosphere.

  16. Crater Copernicus

    NASA Technical Reports Server (NTRS)

    1999-01-01

    HUBBLE SHOOTS THE MOON in a change of venue from peering at the distant universe, NASA's Hubble Space Telescope has taken a look at Earth's closest neighbor in space, the Moon. Hubble was aimed at one of the Moon's most dramatic and photogenic targets, the 58 mile-wide (93 km) impact crater Copernicus. The image was taken while the Space Telescope Imaging Spectrograph(STIS) was aimed at a different part of the moon to measure the colors of sunlight reflected off the Moon. Hubble cannot look at the Sun directly and so must use reflected light to make measurements of the Sun's spectrum. Once calibrated by measuring the Sun's spectrum, the STIS can be used to study how the planets both absorb and reflect sunlight.(upper left)The Moon is so close to Earth that Hubble would need to take a mosaic of 130 pictures to cover the entire disk. This ground-based picture from Lick Observatory shows the area covered in Hubble's photomosaic with the WideField Planetary Camera 2..(center)Hubble's crisp bird's-eye view clearly shows the ray pattern of bright dust ejected out of the crater over one billion years ago, when an asteroid larger than a mile across slammed into the Moon. Hubble can resolve features as small as 600 feet across in the terraced walls of the crater, and the hummock-like blanket of material blasted out by the meteor impact.(lower right)A close-up view of Copernicus' terraced walls. Hubble can resolve features as small as 280 feet across.

  17. Are Ultra-faint Galaxies at z = 6-8 Responsible for Cosmic Reionization? Combined Constraints from the Hubble Frontier Fields Clusters and Parallels

    NASA Astrophysics Data System (ADS)

    Atek, Hakim; Richard, Johan; Jauzac, Mathilde; Kneib, Jean-Paul; Natarajan, Priyamvada; Limousin, Marceau; Schaerer, Daniel; Jullo, Eric; Ebeling, Harald; Egami, Eiichi; Clement, Benjamin

    2015-11-01

    We use deep Hubble Space Telescope imaging of the Frontier Fields to accurately measure the galaxy rest-frame ultraviolet luminosity function (UV LF) in the redshift range z ˜ 6-8. We combine observations in three lensing clusters, A2744, MACS 0416, and MACS 0717, and their associated parallel fields to select high-redshift dropout candidates. We use the latest lensing models to estimate the flux magnification and the effective survey volume in combination with completeness simulations performed in the source plane. We report the detection of 227 galaxy candidates at z = 6-7 and 25 candidates at z ˜ 8. While the total survey area is about 4 arcmin2 in each parallel field, it drops to about 0.6-1 arcmin2 in the cluster core fields because of the strong lensing. We compute the UV LF at z ˜ 7 using the combined galaxy sample and perform Monte Carlo simulations to determine the best-fit Schechter parameters. We are able to reliably constrain the LF down to an absolute magnitude of MUV = -15.25, which corresponds to 0.005 L⋆. More importantly, we find that the faint-end slope remains steep down to this magnitude limit with α =-{2.04}-0.17+0.13. We find a characteristic magnitude of {M}\\star =-{20.89}-0.72+0.60 and log(ϕ⋆) = -{3.54}-0.45+0.48. Our results confirm the most recent results in deep blank fields but extend the LF measurements more than two magnitudes deeper. The UV LF at z ˜ 8 is not very well constrained below MUV = -18 owing to the small number statistics and incompleteness uncertainties. To assess the contribution of galaxies to cosmic reionization, we derive the UV luminosity density at z ˜ 7 by integrating the UV LF down to an observational limit of MUV = -15. We show that our determination of log(ρUV) = 26.2 ± 0.13 (erg s-1 Hz-1 Mpc-3) can be sufficient to maintain reionization with an escape fraction of ionizing radiation of fesc = 10%-15%. Future Hubble Frontier Fields observations will certainly improve the constraints on the UV LF at the epoch of reionization, paving the way to more ambitious programs using cosmic telescopes with the next generation of large aperture telescopes such as the James Webb Space Telescope and the European Extremely Large Telescope. Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with programs 13495, 11386, 13389, and 11689. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. The Hubble Frontier Fields data and the lens models were obtained from the Mikulski Archive for Space Telescopes (MAST). This work utilizes gravitational lensing models produced by PIs Ebeling, Merten, and Zitrin, funded as part of the HST Frontier Fields program conducted by STScI.

  18. A survey of planning and scheduling research at the NASA Ames Research Center

    NASA Technical Reports Server (NTRS)

    Zweben, Monte

    1988-01-01

    NASA Ames Research Center has a diverse program in planning and scheduling. This paper highlights some of our research projects as well as some of our applications. Topics addressed include machine learning techniques, action representations and constraint-based scheduling systems. The applications discussed are planetary rovers, Hubble Space Telescope scheduling, and Pioneer Venus orbit scheduling.

  19. Corporations on Campus.

    ERIC Educational Resources Information Center

    Biddle, Wayne

    1987-01-01

    Examines the effects of increased industrial funding on academic research in science. Highlights the funding arrangements at Carnegie-Mellon University and the Massachusetts Institute of Technology and discusses the impact of university-industry ties. (ML)

  20. New Understanding of Hubble Space Telescope Gyro Current Increase Led to a Method to Save a Failing Gyro Presentation

    NASA Technical Reports Server (NTRS)

    Blumenstock, Kenneth A.

    2017-01-01

    Throughout the history of the Hubble Space Telescope (HST) program, gyro current increases have been observed to occur, often times leading to gyro failure. The explanation was that debris from the surfaces of the gas bearings, with only 1.27 micron clearance, resulted in rotor restriction, which increased friction, torque, and current. However, the rotor restriction theory never could account for the fact that a restart of the gyro would restore the current back to nominal. An effort was made to understand this puzzling gyro behavior after two HST gyros exhibited increased current within the same week in November 2015. A review board was created to resolve these anomalies and generate operational procedures to potentially extend gyro life. A new understanding of gyro current behavior led to implementation of a method that could potentially save a failing gyro.

  1. Long term trending of engineering data for the Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    Cox, Ross M.

    1993-01-01

    A major goal in spacecraft engineering analysis is the detection of component failures before the fact. Trending is the process of monitoring subsystem states to discern unusual behaviors. This involves reducing vast amounts of data about a component or subsystem into a form that helps humans discern underlying patterns and correlations. A long term trending system has been developed for the Hubble Space Telescope. Besides processing the data for 988 distinct telemetry measurements each day, it produces plots of 477 important parameters for the entire 24 hours. Daily updates to the trend files also produce 339 thirty day trend plots each month. The total system combines command procedures to control the execution of the C-based data processing program, user-written FORTRAN routines, and commercial off-the-shelf plotting software. This paper includes a discussion the performance of the trending system and of its limitations.

  2. Minimum Weight Design of a Leaf Spring Tapered in Thickness and Width for the Hubble Space Telescope-Space Support Equipment

    NASA Technical Reports Server (NTRS)

    Rodriguez, P. I.

    1990-01-01

    A linear elastic solution to the problem of minimum weight design of cantilever beams with variable width and depth is presented. The solution shown is for the specific application of the Hubble Space Telescope maintenance mission hardware. During these maintenance missions, delicate instruments must be isolated from the potentially damaging vibration environment of the space shuttle cargo bay during the ascent and descent phases. The leaf springs are designed to maintain the isolation system natural frequency at a level where load transmission to the instruments in a minimum. Nonlinear programming is used for the optimization process. The weight of the beams is the objective function with the deflection and allowable bending stress as the constraint equations. The design variables are the width and depth of the beams at both the free and the fixed ends.

  3. SOFIA Science Imagery

    NASA Image and Video Library

    2017-09-14

    SCI2012_0003: SOFIA mid-infrared image of the planetary nebula Minkowski 2-9 (M2-9), also known as the Butterfly Nebula, compared with a visual-wavelength Hubble Space Telescope image at the same scale and orientation. The nebula is composed of two lobes of gas & dust expelled from a dying star with about the mass of our Sun that is seen at the center of the lobes. The HST image shows mostly ionized gas in the lobes whereas the SOFIA image shows mostly solid grains condensing in the gas. The SOFIA data were obtained during SOFIA's Early Science program in 2011 by a Guest Investigator team led by Michael Werner of Caltech/JPL using the FORCAST camera (P.I.Terry Herter, Cornell University). Credit: SOFIA image, RGB = 37, 24, 20 microns; NASA/DLR/USRA/DSI/FORCAST team/M. Werner et al./A. Helton, J. Rho; HST image: NASA/ESA/NSF/AURA/Hubble Heritage Team/STScI/B. Balick, V. Icke, G. Mellema

  4. The state of the Java universe

    ScienceCinema

    Gosling, James

    2018-05-22

    Speaker Bio: James Gosling received a B.Sc. in computer science from the University of Calgary, Canada in 1977. He received a Ph.D. in computer science from Carnegie-Mellon University in 1983. The title of his thesis was The Algebraic Manipulation of Constraints. He has built satellite data acquisition systems, a multiprocessor version of UNIX®, several compilers, mail systems, and window managers. He has also built a WYSIWYG text editor, a constraint-based drawing editor, and a text editor called Emacs, for UNIX systems. At Sun his early activity was as lead engineer of the NeWS window system. He did the original design of the Java programming language and implemented its original compiler and virtual machine. He has recently been a contributor to the Real-Time Specification for Java.

  5. DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gosling, James

    Speaker Bio: James Gosling received a B.Sc. in computer science from the University of Calgary, Canada in 1977. He received a Ph.D. in computer science from Carnegie-Mellon University in 1983. The title of his thesis was The Algebraic Manipulation of Constraints. He has built satellite data acquisition systems, a multiprocessor version of UNIX®, several compilers, mail systems, and window managers. He has also built a WYSIWYG text editor, a constraint-based drawing editor, and a text editor called Emacs, for UNIX systems. At Sun his early activity was as lead engineer of the NeWS window system. He did the original designmore » of the Java programming language and implemented its original compiler and virtual machine. He has recently been a contributor to the Real-Time Specification for Java.« less

  6. Comet Siding Spring Seen Next to Mars

    NASA Image and Video Library

    2017-12-08

    This composite NASA Hubble Space Telescope Image captures the positions of comet Siding Spring and Mars in a never-before-seen close passage of a comet by the Red Planet, which happened at 2:28 p.m. EDT October 19, 2014. The comet passed by Mars at approximately 87,000 miles (about one-third of the distance between Earth and the Moon). At that time, the comet and Mars were approximately 149 million miles from Earth. The comet image shown here is a composite of Hubble exposures taken between Oct. 18, 8:06 a.m. EDT to Oct. 19, 11:17 p.m. EDT. Hubble took a separate photograph of Mars at 10:37 p.m. EDT on Oct. 18. The Mars and comet images have been added together to create a single picture to illustrate the angular separation, or distance, between the comet and Mars at closest approach. The separation is approximately 1.5 arc minutes, or one-twentieth of the angular diameter of the full Moon. The background starfield in this composite image is synthesized from ground-based telescope data provided by the Palomar Digital Sky Survey, which has been reprocessed to approximate Hubble’s resolution. The solid icy comet nucleus is too small to be resolved in the Hubble picture. The comet’s bright coma, a diffuse cloud of dust enshrouding the nucleus, and a dusty tail, are clearly visible. This is a composite image because a single exposure of the stellar background, comet Siding Spring, and Mars would be problematic. Mars is actually 10,000 times brighter than the comet, and so could not be properly exposed to show detail in the Red Planet. The comet and Mars were also moving with respect to each other and so could not be imaged simultaneously in one exposure without one of the objects being motion blurred. Hubble had to be programmed to track on the comet and Mars separately in two different observations. The images were taken with Hubble’s Wide Field Camera 3. Credit: NASA, ESA, PSI, JHU/APL, STScI/AURA Credit: NASA, ESA, PSI, JHU/APL, STScI/AURA

  7. KSC-08pd2456

    NASA Image and Video Library

    2008-08-18

    CAPE CANAVERAL, Fla. – In the Payload Hazardous Servicing Facility at NASA's Kennedy Space Center, a technicians clean the radiator on the Wide Field Camera 3, or WFC3,that will be installed on NASA's Hubble Space Telescope. The radiator is the "outside" of WFC3 that will be exposed to space. It will expel heat out of Hubble and into space through black body radiation. WFC3 is part of the payload on space shuttle Atlantis' STS-125 mission for the fifth and final Hubble servicing flight to NASA's Hubble Space Telescope. As Hubble enters the last stage of its life, WFC3 will be Hubble's next evolutionary step, allowing Hubble to peer ever further into the mysteries of the cosmos. WFC3 will study a diverse range of objects and phenomena, from young and extremely distant galaxies, to much more nearby stellar systems, to objects within our very own solar system. WFC3 will take the place of Wide Field Planetary Camera 2, which astronauts will bring back to Earth aboard the shuttle. Launch of Atlantis is targeted at 1:34 a.m. EDT Oct. 8. Photo credit: NASA/Amanda Diller

  8. The Fourth Revolution

    ERIC Educational Resources Information Center

    Abelson, Philip H.

    1972-01-01

    Comments on the conclusions of the Carnegie Commission on Higher Education's report, The Fourth Revolution: Instructional Technology in Higher Education,'' and advocates effort in exploiting the new technology and in assessing the possible adverse effects. (AL)

  9. Orbital Debris: Quarterly News, Volume 14, Issue 2

    NASA Technical Reports Server (NTRS)

    Liou, J. C. (Editor); Shoots, Debi (Editor)

    2010-01-01

    This bulletin contains articles from the Orbital Debris Program office. This issue's articles are: "Orbital Debris Success Story --A Decade in the Making", "Old and New Satellite Breakups Identified," "Update on Three Major Debris Clouds," and "MMOD Inspection of the HST Bay 5 Multi-Layer Insulation Panel" about micrometeoroid and orbital debris (MMOD) inspection of the Hubble Space Telescope (HST) insulation panel. A project review is also included (i.e., "Small Debris Observations from the Iridium 33/Cosmos 2251 Collision.") There are also abstra cts of conference papers from the staff of the program office.

  10. Carina Nebula Detail

    NASA Image and Video Library

    2017-12-08

    Carina Nebula Details: Great Clouds Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA) Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html NASA Goddard Space Flight Center is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. Follow us on Twitter Join us on Facebook

  11. High-Redshift SNe with Subaru and HST

    NASA Astrophysics Data System (ADS)

    Rubin, David; Suzuki, Nao; Regnault, Nicolas; Aldering, Gregory; Amanullah, Rahman; Antilogus, Pierre; Astier, Pierre; Barbary, Kyle; Betoule, Marc; Boone, Kyle Robert; Currie, Miles; Deustua, Susana; Doi, Mamoru; Fruchter, Andrew; Goobar, Ariel; Hayden, Brian; Hazenberg, Francois; Hook, Isobel; Huang, Xiaosheng; Jiang, Jian; Kato, Takahiro; Kim, Alex; Kowalski, Marek; Lidman, Chris; Linder, Eric; Maeda, Keiichi; Morokuma, Tomoki; Nordin, Jakob; Pain, Reynald; Perlmutter, Saul; Ruiz-Lapuente, Pilar; Sako, Masao; Myers Saunders, Clare; Spadafora, Anthony L.; Tanaka, Masaomi; Tominaga, Nozomu; Yasuda, Naoki; Yoshida, Naoki

    2018-01-01

    High-redshift type Ia supernovae are crucial for constraining any time variation in dark energy. Here, we present the first discoveries and light curves from the SUbaru Supernovae with Hubble Infrared (SUSHI) program, which combines high-redshift SN discoveries from the Subaru Strategic Program (SSP, as well as other Subaru time) with HST WFC3 IR followup. This program efficiently uses the wide field and high collecting area of Subaru Hyper Suprime-Cam for optical light curves, but still obtains a precision NIR color. We are on track to double the number of well-measured SNe Ia at z > 1.1, triggering on 23 SNe Ia in our first season.

  12. Achieving Agility and Stability in Large-Scale Software Development

    DTIC Science & Technology

    2013-01-16

    temporary team is assigned to prepare layers and frameworks for future feature teams. Presentation Layer Domain Layer Data Access Layer...http://www.sei.cmu.edu/training/ elearning ~ Software Engineering Institute CarnegieMellon

  13. Connected and autonomous vehicles 2040 vision.

    DOT National Transportation Integrated Search

    2014-07-01

    The Pennsylvania Department of Transportation (PennDOT) commissioned a one-year project, Connected and Autonomous : Vehicles 2040 Vision, with researchers at Carnegie Mellon University (CMU) to assess the implications of connected and : autonomous ve...

  14. 21. Engine identified as a 'single cylinder vacuum assist engine ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    21. Engine identified as a 'single cylinder vacuum assist engine for Tod tandem compound engine' showing compressor. - Carnegie Steel-Ohio Works, Steam Engines, 912 Salt Springs Road, Youngstown, Mahoning County, OH

  15. HUBBLE SHOOTS THE MOON

    NASA Technical Reports Server (NTRS)

    2002-01-01

    In a change of venue from peering at the distant universe, NASA's Hubble Space Telescope has taken a look at Earth's closest neighbor in space, the Moon. Hubble was aimed at one of the Moon's most dramatic and photogenic targets, the 58 mile-wide (93 km) impact crater Copernicus. The image was taken while the Space Telescope Imaging Spectrograph (STIS) was aimed at a different part of the moon to measure the colors of sunlight reflected off the Moon. Hubble cannot look at the Sun directly and so must use reflected light to make measurements of the Sun's spectrum. Once calibrated by measuring the Sun's spectrum, the STIS can be used to study how the planets both absorb and reflect sunlight. (upper left) The Moon is so close to Earth that Hubble would need to take a mosaic of 130 pictures to cover the entire disk. This ground-based picture from Lick Observatory shows the area covered in Hubble's photomosaic with the Wide Field Planetary Camera 2.. (center) Hubble's crisp bird's-eye view clearly shows the ray pattern of bright dust ejected out of the crater over one billion years ago, when an asteroid larger than a mile across slammed into the Moon. Hubble can resolve features as small as 600 feet across in the terraced walls of the crater, and the hummock-like blanket of material blasted out by the meteor impact. (lower right) A close-up view of Copernicus' terraced walls. Hubble can resolve features as small as 280 feet across. Credit: John Caldwell (York University, Ontario), Alex Storrs (STScI), and NASA

  16. The Day We Found the Universe: The Little-Known History of How We Came to Understand the Expanding Universe

    NASA Astrophysics Data System (ADS)

    Bartusiak, M.

    2011-09-01

    This will be an overview of the birth of modern cosmology in the 1920s, when the true nature and startling size of the universe was at last revealed. While today Edwin Hubble gets most of the credit, the story is far more complex, involving battles of wills, clever insights, and wrong turns made by a number of investigators before Hubble. The Hubble Space Telescope could easily have had another name if certain events had turned out differently: if Lick Observatory director James Keeler had not prematurely died in 1900 and solved the mystery of the spiral nebulae years earlier; if Lick astronomer Heber Curtis had not taken a promotion in 1920, taking him out of the game; or if astronomer Harlow Shapley, Hubble's nemesis, was not mulishly wedded to a flawed vision of the cosmos. Half the work to prove the universe was expanding was actually performed by Lowell Observatory astronomer Vesto Slipher; Hubble used Slipher's data in 1929 to establish what came to be known as the Hubble Law without citation or acknowledgment, a serious breach of scientific protocol. Even then, Hubble was never a vocal champion of the idea that the universe was expanding. Hubble always coveted an unblemished record: the perfect wife, the perfect scientific findings, the perfect friends. Throughout his life, Hubble claimed that the galaxies fleeing outward were apparent velocities. He wanted to protect his legacy in case a new law of physics was revealed that changed that explanation.

  17. Carnegie Mellon University bioimaging day 2014: Challenges and opportunities in digital pathology

    PubMed Central

    Rohde, Gustavo K.; Ozolek, John A.; Parwani, Anil V.; Pantanowitz, Liron

    2014-01-01

    Recent advances in digital imaging is impacting the practice of pathology. One of the key enabling technologies that is leading the way towards this transformation is the use of whole slide imaging (WSI) which allows glass slides to be converted into large image files that can be shared, stored, and analyzed rapidly. Many applications around this novel technology have evolved in the last decade including education, research and clinical applications. This publication highlights a collection of abstracts, each corresponding to a talk given at Carnegie Mellon University's (CMU) Bioimaging Day 2014 co-sponsored by the Biomedical Engineering and Lane Center for Computational Biology Departments at CMU. Topics related specifically to digital pathology are presented in this collection of abstracts. These include topics related to digital workflow implementation, imaging and artifacts, storage demands, and automated image analysis algorithms. PMID:25250190

  18. Ovarian ectopic pregnancy: diagnosis, treatment, correlation to Carnegie stage 16 and review based on a clinical case.

    PubMed

    Kraemer, Bernhard; Kraemer, Elizabeth; Guengoer, Ersin; Juhasz-Boess, Ingolf; Solomayer, Erich-Franz; Wallwiener, Diethelm; Rajab, Taufiek Konrad

    2009-07-01

    To present a case of a vital ectopic pregnancy after 8 weeks that was located in the right ovary. Case study and literature review. Hospital outpatient clinic. A 29-year-old primigravida presented with lower abdominal pain and mild vaginal bleeding at 8 weeks after her last menstrual period. Wedge resection of the ovary which did not affect subsequent fertility. Conservative treatment options and preservation of patient's reproductive capacity. The embryo was laparoscopically removed in toto and visualized. Therefore, macroscopic correlation to Carnegie stage 16 of development was possible. Approximately 3% of all ectopic pregnancies are located in the ovaries. Preoperative diagnosis of this extremely rare condition is challenging, because the ectopic tumor often resembles cysts of the corpus luteum. At surgery, the trophoblast tissue or the embryo can rarely be visualized completely.

  19. Carnegie Mellon University bioimaging day 2014: Challenges and opportunities in digital pathology.

    PubMed

    Rohde, Gustavo K; Ozolek, John A; Parwani, Anil V; Pantanowitz, Liron

    2014-01-01

    Recent advances in digital imaging is impacting the practice of pathology. One of the key enabling technologies that is leading the way towards this transformation is the use of whole slide imaging (WSI) which allows glass slides to be converted into large image files that can be shared, stored, and analyzed rapidly. Many applications around this novel technology have evolved in the last decade including education, research and clinical applications. This publication highlights a collection of abstracts, each corresponding to a talk given at Carnegie Mellon University's (CMU) Bioimaging Day 2014 co-sponsored by the Biomedical Engineering and Lane Center for Computational Biology Departments at CMU. Topics related specifically to digital pathology are presented in this collection of abstracts. These include topics related to digital workflow implementation, imaging and artifacts, storage demands, and automated image analysis algorithms.

  20. Age determination enhanced by embryonic foot bud and foot plate measurements in relation to Carnegie stages, and the influence of maternal cigarette smoking.

    PubMed

    Lutterodt, M C; Rosendahl, M; Yding Andersen, C; Skouby, S O; Byskov, A G

    2009-08-01

    Reliable age determination of first-trimester human embryos and fetuses is an important parameter for clinical use and basic science. Age determination by ultrasound or morphometric parameters of embryos 4-6 weeks post conception (p.c.) have been questioned, and more accurate methods are required. Data on whether and how maternal smoking and alcohol consumption influence embryonic and fetal foot growth is also lacking. Embryonic tissue from 102 first-trimester legal abortions (aged 35-69 days p.c.) were collected. All women answered a questionnaire concerning smoking and drinking habits, and delivered a urine sample for cotinine analysis. Embryonic age was evaluated by vaginal ultrasound measurements and by post-termination foot length and compared with the Carnegie stages. Foot bud and foot plate were defined and measured as foot length in embryos aged 35-47 days p.c. (range 0.8-2.1 mm). In embryos and fetuses aged 41-69 days p.c., heel-toe length was measured (range 2.5-7.5 mm). We found a significant linear correlation between foot length and age. Morphology of the feet was compared visually with the Carnegie collection, and we found that the mean ages of the two collections correlated well. Foot length was independent of gender, Environmental Tobacco Smoke, maternal smoking and alcohol consumption. Foot length correlated linearly to embryonic and foetal age, and was unaffected by gender, ETS, maternal smoking and alcohol consumption.

  1. A 3D reconstruction of pancreas development in the human embryos during embryonic period (Carnegie stages 15-23).

    PubMed

    Radi, M; Gaubert, J; Cristol-Gaubert, R; Baecker, V; Travo, P; Prudhomme, M; Godlewski, G; Prat-Pradal, D

    2010-01-01

    The goal in this paper was to rebuild a three dimensional (3D) reconstruction of the dorsal and ventral pancreatic buds, in the human embryos, at Carnegie stages 15-23. The early development of the pancreas is studied by tissue observation and reconstruction by a computer-assisted method, using a light micrograph images from consecutive serial sagittal sections (diameter 7 microm) of ten human embryos ranging from Carnegie stages 15-23, CRL 7-27 mm, fixed, dehydrated and embedded in paraffin, were stained alternately with haematoxylin-eosin or Heindenhain'Azan. The images were digitalized by Canon Camera 350 EOS D. The serial views were aligned automatically by software, manual alignment was performed, the data were analysed following segmentation and threshold. The two buds were clearly identified at stage 15. In stage 16, both pancreatic buds were in final position, and begin to merge in stage 17. From stage 18 to the stage 23, surrounding connective tissue differentiated. In the stage 23, the morphology of the pancreas was definitive. The superior portion of the anterior face of the pancreas's head was arising from the dorsal bud. The rest of the head including the uncinate process emanated from the ventral bud. The 3D computer-assisted reconstruction of the human pancreas visualized the relationships between the two pancreatic buds. This explains the disposition and the modality of the components fusion. This embryologic development permits a better understanding of congenital abnormalities.

  2. Dismantling Hubble's Legacy?

    NASA Astrophysics Data System (ADS)

    Way, Michael J.

    2014-01-01

    Edwin Hubble is famous for a number of discoveries that are well known to amateur and professional astronomers, students and even the general public. The origins of three of the most well-known discoveries are examined: The distances to nearby spiral nebulae, the classification of extragalactic-nebulae and the Hubble constant. In the case of the first two a great deal of supporting evidence was already in place, but little credit was given. The Hubble Constant had already been estimated in 1927 by Georges Lemaitre with roughly the same value that Hubble obtained in 1929 using redshifts provided mostly by Vesto M. Slipher. These earlier estimates were not adopted or were forgotten by the astronomical community for complex scientific, sociological and psychological reasons.

  3. The Hubble Deep UV Legacy Survey (HDUV)

    NASA Astrophysics Data System (ADS)

    Montes, Mireia; Oesch, Pascal

    2015-08-01

    Deep HST imaging has shown that the overall star formation density and UV light density at z>3 is dominated by faint, blue galaxies. Remarkably, very little is known about the equivalent galaxy population at lower redshifts. Understanding how these galaxies evolve across the epoch of peak cosmic star-formation is key to a complete picture of galaxy evolution. Here, we present a new HST WFC3/UVIS program, the Hubble Deep UV (HDUV) legacy survey. The HDUV is a 132 orbit program to obtain deep imaging in two filters (F275W and F336W) over the two CANDELS Deep fields. We will cover ~100 arcmin2 sampling the rest-frame far-UV at z>~0.5, this will provide a unique legacy dataset with exquisite HST multi-wavelength imaging as well as ancillary HST grism NIR spectroscopy for a detailed study of faint, star-forming galaxies at z~0.5-2. The HDUV will enable a wealth of research by the community, which includes tracing the evolution of the FUV luminosity function over the peak of the star formation rate density from z~3 down to z~0.5, measuring the physical properties of sub-L* galaxies, and characterizing resolved stellar populations to decipher the build-up of the Hubble sequence from sub-galactic clumps. This poster provides an overview of the HDUV survey and presents the reduced data products and catalogs which will be released to the community, reaching down to 27.5-28.0 mag at 5 sigma. By directly sampling the rest-frame far-UV at z>~0.5, this will provide a unique legacy dataset with exquisite HST multi-wavelength imaging as well as ancillary HST grism NIR spectroscopy for a detailed study of faint, star-forming galaxies at z~0.5-2. The HDUV will enable a wealth of research by the community, which includes tracing the evolution of the FUV luminosity function over the peak of the star formation rate density from z~3 down to z~0.5, measuring the physical properties of sub-L* galaxies, and characterizing resolved stellar populations to decipher the build-up of the Hubble sequence from sub-galactic clumps. This poster provides an overview of the HDUV survey and presents reduced data products and catalogs which will be released to the community.

  4. A Unique test for Hubble's new Solar Arrays

    NASA Astrophysics Data System (ADS)

    2000-10-01

    In mid-October, a team from the European Space Agency (ESA) and NASA will perform a difficult, never-before-done test on one of the Hubble Space Telescope's new solar array panels. Two of these panels, or arrays, will be installed by astronauts in November 2001, when the Space Shuttle Columbia visits Hubble on a routine service mission. The test will ensure that the new arrays are solid and vibration free before they are installed on orbit. The test will be conducted at ESA's European Space Research and Technology Center (ESTEC) in Noordwijk, The Netherlands. Because of the array's size, the facility's special features, and ESA's longstanding experience with Hubble's solar arrays, ESTEC is the only place in the world the test can be performed. This test is the latest chapter in a longstanding partnership between ESA and NASA on the Hubble Space Telescope. The Large Space Simulator at ESTEC, ESA's world-class test facility, features a huge vacuum chamber containing a bank of extremely bright lights that simulate the Sun's intensity - including sunrise and sunset. By exposing the solar wing to the light and temperature extremes of Hubble's orbit, engineers can verify how the new set of arrays will act in space. Hubble orbits the Earth once every 90 minutes. During each orbit, the telescope experiences 45 minutes of searing sunlight and 45 minutes of frigid darkness. This test will detect any tiny vibrations, or jitters, caused by these dramatic, repeated changes. Even a small amount of jitter can affect Hubble's sensitive instruments and interfere with observations. Hubble's first set of solar arrays experienced mild jitter and was replaced in 1993 with a much more stable pair. Since that time, advances in solar cell technology have led to the development of even more efficient arrays. In 2001, NASA will take advantage of these improvements, by fitting Hubble with a third-generation set of arrays. Though smaller, this new set generates more power than the previous pairs. The arrays use high efficiency solar cells and an advanced structural system to support the solar panels. Unlike the earlier sets, which roll up like window shades, the new arrays are rigid. ESA provided Hubble's first two sets of solar arrays, and built and tested the motors and electronics of the new set provided by NASA Goddard Space Flight Center. Now, this NASA/ESA test has benefits that extend beyond Hubble to the world-wide aerospace community. It will greatly expand basic knowledge of the jitter phenomenon. Engineers across the globe can apply these findings to other spacecraft that are subjected to regular, dramatic changes in sunlight and temperature. Note to editors The Hubble Project The Hubble Space Telescope is a project of international co-operation between the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA). The partnership agreement between ESA and NASA was signed on 7 October 1977. ESA has provided two pairs of solar panels and one of Hubble's scientific instruments (the Faint Object Camera), as well as a number of other components and supports NASA during routine Servicing Missions to the telescope. In addition, 15 European scientists are working at the Space Telescope Science Institute in Baltimore (STScI), which is responsible for the scientific operation of the Hubble Observatory and is managed by the Association of Universities for Research in Astronomy (AURA) for NASA. In return, European astronomers have guaranteed access to 15% of Hubble's observing time. The Space Telescope European Coordinating Facility (ST-ECF) hosted at the European Southern Observatory (ESO) in Garching bei München, Germany, supports European Hubble users. ESA and ESO jointly operate the ST-ECF.

  5. HUBBLE UNCOVERS MYSTERY OBJECTS IN THE DENSE CORE OF A NEARBY STAR CLUSTER

    NASA Technical Reports Server (NTRS)

    2002-01-01

    Piercing the heart of a glittering swarm of stars, NASA's sharp-eyed Hubble Space Telescope unveils the central region of the globular cluster M22, a 12- to 14-billion-year-old grouping of stars in the constellation Sagittarius. The telescope's view of the cluster's core measures 3.3 light-years across. The stars near the cluster's core are 100,000 times more numerous than those in the Sun's neighborhood. Buried in the glow of starlight are about six 'mystery objects,' which astronomers estimate are no larger than one quarter the mass of the giant planet Jupiter, the solar system's heftiest planet. The mystery objects are too far and dim for Hubble to see directly. Instead, the orbiting observatory detected these unseen celestial bodies by looking for their gravitational effects on the light from far distant stars. In this case, the stars are far beyond the cluster in the galactic bulge, about 30,000 light-years from Earth at the center of the Milky Way Galaxy. M22 is 8,500 light-years away. The invisible objects betrayed their presence by bending the starlight gravitationally and amplifying it, a phenomenon known as microlensing. From February 22 to June 15, 1999, Hubble's Wide Field and Planetary Camera 2 looked through this central region and monitored 83,000 stars. During that time the orbiting observatory recorded six unexpectedly brief microlensing events. In each case a background star jumped in brightness for less than 20 hours before dropping back to normal. These transitory spikes in brightness mean that the object passing in front of the star must have been much smaller than a normal star. Hubble also detected one clear microlensing event. In that observation a star appeared about 10 times brighter over an 18-day span before returning to normal. Astronomers traced the leap in brightness to a dwarf star in the cluster floating in front of the background star. The inset photo shows the entire globular cluster of about 10 million stars. M22 is about 60 light-years wide. The image was taken in June 1995 by the Burrell Schmidt telescope at the Case Western Reserve University's Warner and Swasey Observatory on Kitt Peak in Arizona. This release is issued jointly by NASA and ESA. Credits for Hubble image: NASA, Kailash Sahu, Stefano Casertano, Mario Livio, Ron Gilliland (Space Telescope Science Institute), Nino Panagia (European Space Agency/Space Telescope Science Institute), Michael Albrow and Mike Potter (Space Telescope Science Institute) Credits for ground-based image: Nigel A.Sharp, REU program/AURA/NOAO/NSF

  6. Hubble Captures Celestial Fireworks Within the Large Magellanic Cloud

    NASA Technical Reports Server (NTRS)

    2000-01-01

    This is a color Hubble Space Telescope (HST) heritage image of supernova remnant N49, a neighboring galaxy, that was taken with Hubble's Wide Field Planetary Camera 2. Color filters were used to sample light emitted by sulfur, oxygen, and hydrogen. The color image was superimposed on a black and white image of stars in the same field also taken with Hubble. Resembling a fireworks display, these delicate filaments are actually sheets of debris from a stellar explosion.

  7. History of Hubble Space Telescope (HST)

    NASA Image and Video Library

    2000-07-01

    This is a color Hubble Space Telescope (HST) heritage image of supernova remnant N49, a neighboring galaxy, that was taken with Hubble's Wide Field Planetary Camera 2. Color filters were used to sample light emitted by sulfur, oxygen, and hydrogen. The color image was superimposed on a black and white image of stars in the same field also taken with Hubble. Resembling a fireworks display, these delicate filaments are actually sheets of debris from a stellar explosion.

  8. The (Historical) Search for Planets Orbiting Proxima Centauri

    NASA Astrophysics Data System (ADS)

    Kohler, Susanna

    2016-08-01

    The European Southern Observatory (ESO) is widely expected to address the reportsofthe discovery of a planet orbiting our nearest stellar neighbor, Proxima Centauri, today. Due to its proximity 4.25 light-years away this red dwarf star has been a prime target for exoplanet searches throughout the last couple decades.Hubble image of Proxima Centauri, our nearest stellar neighbor. [ESA/Hubble]In anticipation of ESOspress conference this afternoon, lets take a look at someof the past work in the search for planetary companions around Proxima Centauri.The Early Years of Exploring Proxima CentauriProxima Centauri was discovered by astronomer Robert Innes in 1915. Studies of this star over the next eighty years primarily focused on better understanding its orbital motion (is it part of the Alpha Centauri star system?) and its flaring nature. But in the 1990s, after the detection of the first exoplanets, Proxima Centauri became a target for its potential to host planet-mass companions.Top: Images of Proxima Centauri on two different days from Hubbles FOS instrument. The bar across the center is an occulter that partially blocks the light from Proxima Centauri. Middle: Reconstructed images allowing a closer look at a moving feature identified by the authors as a possible companion. Bottom: diagram of the position of the planet candidate (box) relative to Proxima Centauri (star) in the two frames. [Schultz et al. 1998]1990s: A Possible Planet Detected With Hubble?In January 1998, a paper led by A.B. Schultz (STScI) reported the possible visual detection of a planetary companion to Proxima Centauri. Observations from Hubbles Faint Object Spectrograph, which was being used as a coronagraphic camera, revealed excess light that could be interpreted as a substellar object located ~0.5 AU from Proxima Centauri, a small separation that could imply either a short (~1 yr) period or a highly eccentric orbit.But follow-up observations led by David Golimowski (Johns Hopkins University) were unable to detect this proposed planet. These observations made by direct imaging with Hubbles Wide Field Planetary Camera 2 found no evidence of a companion located 0.121.1 AU from Proxima Centauri.In addition, an astrometric study led by G. Fritz Benedict (McDonald Observatory) the following year also didnt find any evidence for the proposed companion. Along with prior radial velocity measurements, the astrometry in this study ruled out all companions to Proxima Centauri with a mass of more than 0.8 Jupiter masses and periods between 1 and 1000 days.Increased Capabilities in Recent YearsWith increasing resolution and sensitivity of instruments, as well as better stellar modeling and increased noise-reduction strategies, we are now more likely than ever to be able to detect a planet orbiting Proxima Centauri. Therefore, our continued non-detections have been placing ever more stringent limits on the mass and orbital properties of a hypothetical companion.In 2014, as part of a long-term study of the solar neighborhood, a team led by John Lurie (University of Washington) published the results of a nearly 13-year campaign that used the Cerro Tololo Inter-American Observatory to obtain astrometric measurements for Proxima Centauri. This detailed study ruled out the possibility of Jupiter-mass companions at orbital periods of 212 years.Radial-velocity measurements of Proxima Centauri from a 2012 study using HARPS-TERRA. No promising signals of companions were found. [Anglada-Escud and Butler 2012]One of the most advanced instruments currently in the radial-velocity planet search is a spectrometer called the High Accuracy Radial velocity Planet Searcher (HARPS), operated by ESOin La Silla Observatory, Chile. In a study from 2012 led by Guillem Anglada-Escud (Carnegie Institution of Washington), the team described new data analysis algorithms being used with HARPS. The authors used Proxima Centauri as a test case, finding only a very marginal signal with a period of 5.6 days. The signals lack of significance led them to conclude that, unfortunately, no promising signals are yet detected on Proxima Cen.These studies among others throughout the last couple decades have placed strict limitations on the mass and orbit of a potential planetary companion to our nearest stellar neighbor. It will be interesting to see what ESO announces this afternoon, and how it fits into the context of these past studies of Proxima Centauri!CitationsA. B. Schultz et al 1998 AJ 115 345. doi:10.1086/300176David A. Golimowski and Daniel J. Schroeder 1998 AJ 116 440. doi:10.1086/300437G. Fritz Benedict et al 1999 AJ 118 1086. doi:10.1086/300975John C. Lurie et al 2014 AJ 148 91. doi:10.1088/0004-6256/148/5/91Guillem Anglada-Escud and R. Paul Butler 2012 ApJS 200 15. doi:10.1088/0067-0049/200/2/15

  9. Venus Cloud Tops Viewed by Hubble

    NASA Image and Video Library

    1999-05-18

    Venus Cloud Tops Viewed by Hubble. This is a NASA Hubble Space Telescope ultraviolet-light image of the planet Venus, taken on January 24 1995, when Venus was at a distance of 70.6 million miles 113.6 million kilometers from Earth.

  10. STS-61 Space Shuttle mission report

    NASA Technical Reports Server (NTRS)

    Fricke, Robert W., Jr.

    1994-01-01

    The STS-61 Space Shuttle Program Mission Report summarizes the Hubble Space Telescope (HST) servicing mission as well as the Orbiter, External Tank (ET), Solid Rocket Booster (SRB), Redesigned Solid Rocket Motor (RSRM), and the Space Shuttle main engine (SSME) systems performance during the fifty-ninth flight of the Space Shuttle Program and fifth flight of the Orbiter vehicle Endeavour (OV-105). In addition to the Orbiter, the flight vehicle consisted of an ET designated as ET-60; three SSME's which were designated as serial numbers 2019, 2033, and 2017 in positions 1, 2, and 3, respectively; and two SRB's which were designated BI-063. The RSRM's that were installed in each SRB were designated as 360L023A (lightweight) for the left SRB, and 360L023B (lightweight) for the right SRB. This STS-61 Space Shuttle Program Mission Report fulfills the Space Shuttle Program requirement as documented in NSTS 07700, Volume 8, Appendix E. That document requires that each major organizational element supporting the Program report the results of its hardware evaluation and mission performance plus identify all related in-flight anomalies. The primary objective of the STS-61 mission was to perform the first on-orbit servicing of the Hubble Space Telescope. The servicing tasks included the installation of new solar arrays, replacement of the Wide Field/Planetary Camera I (WF/PC I) with WF/PC II, replacement of the High Speed Photometer (HSP) with the Corrective Optics Space Telescope Axial Replacement (COSTAR), replacement of rate sensing units (RSU's) and electronic control units (ECU's), installation of new magnetic sensing systems and fuse plugs, and the repair of the Goddard High Resolution Spectrometer (GHRS). Secondary objectives were to perform the requirements of the IMAX Cargo Bay Camera (ICBC), the IMAX Camera, and the Air Force Maui Optical Site (AMOS) Calibration Test.

  11. KSC-08pd2455

    NASA Image and Video Library

    2008-08-18

    CAPE CANAVERAL, Fla. – In the Payload Hazardous Servicing Facility at NASA's Kennedy Space Center, a technician cleans the edge of the radiator on the Wide Field Camera 3, or WFC3,that will be installed on NASA's Hubble Space Telescope. The radiator is the "outside" of WFC3 that will be exposed to space. It will expel heat out of Hubble and into space through black body radiation. WFC3 is part of the payload on space shuttle Atlantis' STS-125 mission for the fifth and final Hubble servicing flight to NASA's Hubble Space Telescope. As Hubble enters the last stage of its life, WFC3 will be Hubble's next evolutionary step, allowing Hubble to peer ever further into the mysteries of the cosmos. WFC3 will study a diverse range of objects and phenomena, from young and extremely distant galaxies, to much more nearby stellar systems, to objects within our very own solar system. WFC3 will take the place of Wide Field Planetary Camera 2, which astronauts will bring back to Earth aboard the shuttle. Launch of Atlantis is targeted at 1:34 a.m. EDT Oct. 8. Photo credit: NASA/Amanda Diller

  12. The critical role of culture and environment as determinants of women's participation in computer science

    NASA Astrophysics Data System (ADS)

    Frieze, Carol

    This thesis proposes the need for, and illustrates, a new approach to how we think about, and act on, issues relating to women's participation, or lack of participation, in computer science (CS). This approach is based on a cultural perspective arguing that many of the reasons for women entering---or not entering---CS programs have little to do with gender and a lot to do with environment and culture. Evidence for this approach comes primarily from a qualitative, research study, which shows the effects of changes in the micro-culture on CS undergraduates at Carnegie Mellon, and from studies of other cultural contexts that illustrate a "Women-CS fit". We also discuss the interventions that have been crucial to the evolution of this specific micro-culture. Our argument goes against the grain of many gender and CS studies which conclude that the reasons for women's low participation in CS are based in gender --and particularly in gender differences in how men and women relate to the field. Such studies tend to focus on gender differences and recommend accommodating (what are perceived to be) women's different ways of relating to CS. This is often interpreted as contextualizing the curriculum to make it "female-friendly". The CS curriculum at Carnegie Mellon was not contextualized to be "female-friendly". Nevertheless, over the past few years, the school has attracted and graduated well above the US national average for women in undergraduate CS programs. We argue that this is due in large part to changes in the culture and environment of the department. As the environment has shifted from an unbalanced to a more balanced environment (balanced in terms of gender, breadth of student personalities, and professional support for women) the way has been opened for a range of students, including a significant number of women, to participate, and be successful, in the CS major. Our research shows that as men and women inhabit, and participate in, a more balanced environment, perceived gender differences start to dissolve and we see men and women displaying many gender similarities in how they relate to CS.

  13. Achieving Agility and Stability in Large-Scale Software Development

    DTIC Science & Technology

    2013-01-16

    temporary team is assigned to prepare layers and frameworks for future feature teams. Presentation Layer Domain Layer Data Access Layer Framework...http://www.sei.cmu.edu/training/ elearning ~ Software Engineering Institute CarnegieMellon

  14. Carbon Monoxide Monitor for Automobile Passenger Compartment

    DOT National Transportation Integrated Search

    1991-07-01

    This document reports the results of the study conducted by the Carnegie Mellon Research Institute (CMRI) to evaluate its recently developed metal oxide semiconductor (MOS) gas sensor technology for applications in the automobile environment. The spe...

  15. Developing Effective Performance Measures

    DTIC Science & Technology

    2014-10-14

    University When Performance Measurement Goes Bad Laziness Vanity Narcissism Too Many Pettiness Inanity 52 Developing Effective...Kasunic, October 14, 2014 © 2014 Carnegie Mellon University Narcissism Measuring performance from the organization’s point of view, rather than from

  16. 12. A DETAIL VIEW OF THE NORTHEASTERN END POST, LOOKING ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    12. A DETAIL VIEW OF THE NORTHEASTERN END POST, LOOKING SOUTH, SHOWING THE MANUFACTURER'S MARK, 'CARNEGIE'. - Wells County Bridge No. 74, Spanning Rock Creek Ditch at County Road 400, Bluffton, Wells County, IN

  17. Computers, Electronic Networking and Education: Some American Experiences.

    ERIC Educational Resources Information Center

    McConnell, David

    1991-01-01

    Describes new developments in distributed educational computing at Massachusetts Institute of Technology (MIT, "Athena"), Carnegie Mellon University ("Andrew"), Brown University "Intermedia"), Electronic University Network (California), Western Behavioral Sciences Institute (California), and University of California,…

  18. 20. Engine identified as a 'single cylinder vacuum assist engine ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    20. Engine identified as a 'single cylinder vacuum assist engine for the Tod tandem compound engine' showing crank end. - Carnegie Steel-Ohio Works, Steam Engines, 912 Salt Springs Road, Youngstown, Mahoning County, OH

  19. 19. Engine identified as a single cylinder vacuum assist engine ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    19. Engine identified as a single cylinder vacuum assist engine for the Filer and Stowell 15-inch continuous mill. - Carnegie Steel-Ohio Works, Steam Engines, 912 Salt Springs Road, Youngstown, Mahoning County, OH

  20. NASA Hubble Space Telescope (HST) Research Project Capstone Even

    NASA Image and Video Library

    2014-05-05

    John Grunsfeld, NASA Associate Administrator for the Science Mission Directorate, speaks to students from Mapletown Jr/Sr High School and Margaret Bell Middle School about his experiences on the final space shuttle servicing mission to the Hubble Space Telescope during the NASA Hubble Space Telescope (HST) Research Project Capstone Event in the James E. Webb Auditorium at NASA Headquarters on Monday, May 5, 2014. Grunsfeld flew on three of the five servicing missions to the Hubble Space Telescope. Photo Credit: (NASA/Joel Kowsky)

  1. Saturn's Rings in Ultraviolet Light

    NASA Image and Video Library

    2017-12-08

    Saturn's Rings in Ultraviolet Light Credit: NASA and E. Karkoschka (University of Arizona) The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html

  2. Space Shuttle Projects

    NASA Image and Video Library

    2002-03-07

    STS-109 Astronaut Michael J. Massimino, mission specialist, perched on the Shuttle's robotic arm, is preparing to install the Electronic Support Module (ESM) in the aft shroud of the Hubble Space telescope (HST), with the assistance of astronaut James H. Newman (out of frame). The module will support a new experimental cooling system to be installed during the next day's fifth and final space walk of the mission. That cooling system is designed to bring the telescope's Near-Infrared Camera and Multi Spectrometer (NICMOS) back to life the which had been dormant since January 1999 when its original coolant ran out. The Space Shuttle Columbia STS-109 mission lifted off March 1, 2002 with goals of repairing and upgrading the Hubble Space Telescope (HST). The Marshall Space Flight Center in Huntsville, Alabama had the responsibility for the design, development, and construction of the HST, which is the most powerful and sophisticated telescope ever built. In addition to the installation of the experimental cooling system for the Hubble's Near-Infrared Camera and NICMOS, STS-109 upgrades to the HST included replacement of the solar array panels, replacement of the power control unit (PCU), and replacement of the Faint Object Camera (FOC) with a new advanced camera for Surveys (ACS). Lasting 10 days, 22 hours, and 11 minutes, the STS-109 mission was the 108th flight overall in NASA's Space Shuttle Program.

  3. SPECTROSCOPIC CONFIRMATION OF FAINT LYMAN BREAK GALAXIES NEAR REDSHIFT FIVE IN THE HUBBLE ULTRA DEEP FIELD

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Rhoads, James E.; Malhotra, Sangeeta; Cohen, Seth

    We present the faintest spectroscopically confirmed sample of z {approx} 5 Lyman break galaxies (LBGs) to date. The sample is based on slitless grism spectra of the Hubble Ultra Deep Field region from the Grism ACS Program for Extragalactic Science (GRAPES) and Probing Evolution and Reionization Spectroscopically (PEARS) projects, using the G800L grism on the Hubble Space Telescope Advanced Camera for Surveys. We report here confirmations of 39 galaxies, preselected as candidate LBGs using photometric selection criteria. We compare a 'traditional' V-dropout selection, based on the work of Giavalisco et al., to a more liberal one (with V - imore » > 0.9), and find that the traditional criteria are about 64% complete and 81% reliable. We also study the Ly{alpha} emission properties of our sample. We find that Ly{alpha} emission is detected in {approx}1/4 of the sample, and that the liberal V-dropout color selection includes {approx}55% of previously published line-selected Ly{alpha} sources. Finally, we examine our stacked two-dimensional spectra. We demonstrate that strong, spatially extended ({approx}1'') Ly{alpha} emission is not a generic property of these LBGs, but that a modest extension of the Ly{alpha} photosphere (compared to the starlight) may be present in those galaxies with prominent Ly{alpha} emission.« less

  4. KSC-08pd2457

    NASA Image and Video Library

    2008-08-18

    CAPE CANAVERAL, Fla. – In the Payload Hazardous Servicing Facility at NASA's Kennedy Space Center, a technician checks the pick-off mirror on the Wide Field Camera 3, or WFC3, that will be installed on NASA's Hubble Space Telescope. WFC3 is part of the payload on space shuttle Atlantis' STS-125 mission for the fifth and final Hubble servicing flight to Hubble. As Hubble enters the last stage of its life, WFC3 will be Hubble's next evolutionary step, allowing Hubble to peer ever further into the mysteries of the cosmos. WFC3 will study a diverse range of objects and phenomena, from young and extremely distant galaxies, to much more nearby stellar systems, to objects within our very own solar system. WFC3 will take the place of Wide Field Planetary Camera 2, which astronauts will bring back to Earth aboard the shuttle. Launch of Atlantis is targeted at 1:34 a.m. EDT Oct. 8. Photo credit: NASA/Amanda Diller

  5. A Prototype Tactile Sensor Array.

    DTIC Science & Technology

    1982-09-15

    Active Touch Sensing. Technical Report, MIT Artificial Inteligence Laboratory, 1981. (9] Larcombe, M. Carbon Fibre Tactile Sensors. Technical Report...thesis, Carnegie-Mellon University, 1981. [13] Purbrick, John A. A Force Transducer Employing Conductive Silicone Rubber. Technical Report, MIT Artificial

  6. Wales as a Setting for Children's Fantasy.

    ERIC Educational Resources Information Center

    Kiefer, Barbara Z.

    1982-01-01

    Examines three works of fantasy that have been awarded the Newbery or Carnegie Medal during the last 15 years ("The High King,""The Owl Service," and "The Grey King") and that have used Wales as their setting. (HOD)

  7. Information Processing Research

    DTIC Science & Technology

    1979-06-01

    quantitative shape recovery. For the qualitative shape recovery we use a model of the Origami world (Kanade, 1978), together with edge profiles of...Workshop. Carnegie-Mellon University, Computer Science Department, Pittsburgh, PA, November, 1978. Kanade, T. A theory of origami world. Technical

  8. Impact of aerosols, dust, water vapor and clouds on fair weather PG and implications for the Carnegie curve

    NASA Astrophysics Data System (ADS)

    Kourtidis, Konstantinos; Georgoulias, Aristeidis

    2017-04-01

    We studied the impact of anthropogenic aerosols, fine mode natural aerosols, Saharan dust, atmospheric water vapor, cloud fraction, cloud optical depth and cloud top height on the magnitude of fair weather PG at the rural station of Xanthi. Fair weather PG was measured in situ while the other parameters were obtained from the MODIS instrument onboard the Terra and Aqua satellites. All of the above parameteres were found to impact fair weather PG magnitude. Regarding aerosols, the impact was larger for Saharan dust and fine mode natural aerosols whereas regarding clouds the impact was larger for cloud fraction while less than that of aerosols. Water vapour and ice precipitable water were also found to influence fair weather PG. Since aerosols and water are ubiquitous in the atmosphere and exhibit large spatial and temporal variability, we postulate that our understanding of the Carnegie curve might need revision.

  9. Morphogenesis of the human excretory lacrimal system

    PubMed Central

    de la Cuadra-Blanco, C; Peces-Peña, M D; Jáñez-Escalada, L; Mérida-Velasco, J R

    2006-01-01

    The aim of this study was to determine the principal developmental stages in the formation of the excretory lacrimal system in humans and to establish its morphogenetic period. The study was performed using light microscopy on serial sections of 51 human specimens: 33 embryos and 18 fetuses ranging from 8 to 137 mm crown–rump length (CR; 5–16 weeks of development). Three stages were identified in the morphogenesis of the excretory lacrimal system: (1) the formative stage of the lacrimal lamina (Carnegie stages 16–18); (2) the formative stage of the lacrimal cord (Carnegie stages 19–23); and (3) the maturative stage of the excretory lacrimal system, from the 9th week of development onward. A three-dimensional reconstruction of the excretory lacrimal system was performed from serial sections of an embryo at the end of the embryonic period (27 mm CR). PMID:16879594

  10. Hubble's deepest view ever of the Universe unveils earliest galaxies

    NASA Astrophysics Data System (ADS)

    2004-03-01

    Hubble sees galaxies galore hi-res Size hi-res: 446 kb Credits: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team Hubble sees galaxies galore Galaxies, galaxies everywhere - as far as the NASA/ESA Hubble Space Telescope can see. This view of nearly 10,000 galaxies is the deepest visible-light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy-studded view represents a ‘deep’ core sample of the universe, cutting across billions of light-years. Hubble reveals galactic drama hi-res Size hi-res: 879 kb Credits: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team Hubble reveals galactic drama A galactic brawl. A close encounter with a spiral galaxy. Blue wisps of galaxies. These close-up snapshots of galaxies in the Hubble Ultra Deep Field reveal the drama of galactic life. Here three galaxies just below centre are enmeshed in battle, their shapes distorted by the brutal encounter. Hubble reveals galactic drama hi-res Size hi-res: 886 kb Credits: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team Hubble reveals galactic drama A galactic brawl. A close encounter with a spiral galaxy. Blue wisps of galaxies. These close-up snapshots of galaxies in the Hubble Ultra Deep Field reveal the drama of galactic life. Here three galaxies just below centre are enmeshed in battle, their shapes distorted by the brutal encounter. Hubble reveals galactic drama hi-res Size hi-res: 892 kb Credits: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team Hubble reveals galactic drama A galactic brawl. A close encounter with a spiral galaxy. Blue wisps of galaxies. These close-up snapshots of galaxies in the Hubble Ultra Deep Field reveal the drama of galactic life. The galaxies in this panel were plucked from a harvest of nearly 10,000 galaxies in the Ultra Deep Field, the deepest visible-light image of the cosmos. This historic new view is actually made up by two separate images taken by Hubble's Advanced Camera for Surveys (ACS) and the Near Infrared Camera and Multi-object Spectrometer (NICMOS). Both images reveal some galaxies that are too faint to be seen by ground-based telescopes, or even in Hubble's previous faraway looks, called the Hubble Deep Fields (HDFs), taken in 1995 and 1998. The HUDF field contains an estimated 10,000 galaxies in a patch of sky just one-tenth the diameter of the full Moon. Besides the rich harvest of classic spiral and elliptical galaxies, there is a zoo of oddball galaxies littering the field. Some look like toothpicks; others like links on a bracelet. A few appear to be interacting. Their strange shapes are a far cry from the majestic spiral and elliptical galaxies we see today. These oddball galaxies chronicle a period when the Universe was more chaotic. Order and structure were just beginning to emerge. The combination of ACS and NICMOS images will be used to search for galaxies that existed between 400 and 800 million years after the Big Bang (in cosmological terms this corresponds to a 'redshift' range of 7 to 12). Astronomers around the world will use these data to understand whether in this very early stages the Universe appears to be the same as it did when the cosmos was between 1000 and 2000 million years old. Hubble's ACS allows astronomers to see galaxies two to four times fainter than Hubble could view previously, but the NICMOS sees even farther than the ACS. The NICMOS reveals the farthest galaxies ever seen because the expanding Universe has stretched their light into the near-infrared portion of the spectrum. The ACS uncovered galaxies that existed 800 million years after the Big Bang (at a redshift of 7). But the NICMOS might have spotted galaxies that lived just 400 million years after the birth of the cosmos (at a redshift of 12). Just like the previous HDFs, the new data are expected to galvanise the astronomical community and lead to dozens of research papers that will offer new insights into the birth and evolution of galaxies. This will hold the record as the deepest-ever view of the Universe until ESA together with NASA launches the James Webb Space Telescope in 2011. Notes for editors More information, images, animations and interactive zoomable images are available from http://www.spacetelescope.org/news/html/heic0406.html The Hubble Space Telescope is a project of international cooperation between ESA and NASA. Image credit: NASA, ESA, S. Beckwith (STScI) and the HUDF Team

  11. Optimal Dictionaries for Sparse Solutions of Multi-frame Blind Deconvolution

    DTIC Science & Technology

    2014-09-01

    object is the Hubble Space Telescope (HST). As stated above, the dictionary training used the first 100 of the total of the simulated PSFs. The second set...diffraction-limited Hubble image and HubbleRE is the reconstructed image from the 100 simulated atmospheric turbulence degraded images of the HST

  12. Upgraded Hubble Space Telescope Images

    NASA Image and Video Library

    2009-09-08

    David Leckrone, senior project scientist for Hubble at NASA's Goddard Space Flight Center in Greenbelt, Md. discusses newly released images from NASA's Hubble Space Telescope Wednesday, Sept. 9, 2009 at NASA Headquarters in Washington. The images were from four of the telescopes' six operating science instruments. Photo Credit: (NASA/Bill Ingalls)

  13. Repairing Hubble Exhibit Reception

    NASA Image and Video Library

    2014-04-23

    Individuals in attendance who had a hand in the development or servicing of the Hubble Space Telescope pose for a group photo at an event unveiling a new exhibit featuring Hubble's Corrective Optics Space Telescope Axial Replacement (COSTAR) and the WFPC2 on Wednesday, April 23, 2014 at the Smithsonian National Air and Space Museum in Washington, DC. COSTAR and WFPC2 were installed in Hubble during the first space shuttle servicing mission in 1993 and returned to Earth on the fifth and final servicing mission in 2009. Photo Credit: (NASA/Joel Kowsky)

  14. A Scientific Revolution: the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2011-01-01

    Astronomy is going through a scientific revolution, responding to a flood of data from the Hubble Space Telescope, other space missions, and large telescopes on the ground. In this talk, I will discuss some of the most important astronomical discoveries of the last 10 years, and the role that space telescopes have played in those discoveries. The next decade looks equally bright with the newly refurbished Hubble and the promise of its successor, the James Webb Space Telescope. I will describe how Hubble was upgraded and how and why we are building Webb.

  15. A Scientific Revolution: The Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan

    2011-01-01

    Astronomy is going through a scientific revolution, responding to a flood of data from the Hubble Space Telescope, other space missions, and large telescopes on the ground. In this talk, I will discuss some of the most important astronomical discoveries of the last 10 years, and the role that space telescopes have played in those discoveries. The next decade looks equally bright with the newly refurbished Hubble and the promise of its successor, the James Webb Space Telescope. I will describe how Hubble was upgraded and how and why we are building Webb.

  16. A Scientific Revolution: The Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2009-01-01

    Astronomy is going through a scientific revolution, responding to a flood of data from the Hubble Space Telescope, other space missions, and large telescopes on the ground. In this talk, I will discuss the top 10 astronomical discoveries of the last 10 years, and the role that space telescopes have played in those discoveries. The next decade looks equally bright with the newly refurbished Hubble and the promise of its successor, the James Webb Space Telescope. I will describe how Hubble was upgraded and how and why we are building Webb.

  17. A Scientific Revolution: the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2012-01-01

    Astronomy is going through a scientific revolution, responding to a flood of data from the Hubble Space Telescope, other space missions, and large telescopes on the ground. In this talk, I will discuss some of the most important astronomical discoveries of the last IO years, and the role that space telescopes have played in those discoveries. The next decade looks equally bright with the newly refurbished Hubble and the promise of its successor, the James Webb Space Telescope. I will describe how Hubble was upgraded and how and why we are building Webb.

  18. Finding our Origins with the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan P.

    2009-01-01

    NASA is planning a successor to the Hubble Space Telescope designed to study the origins of galaxies, stars, planets and life in the universe. In this talk, Dr. Gardner will discuss the origin and evolution of galaxies, beginning with the Big Bang and tracing what we have learned with Hubble through to the present day. He will show that results from studies with Hubble have led to plans for its successor, the James Webb Space Telescope. Webb is scheduled to launch in 2014, and is designed to find the first galaxies that formed in the distant past and to penetrate the dusty clouds of gas where stars are still forming today. He will compare Webb to Hubble, and discuss recent progress in the construction of the observatory.

  19. Light Echo

    NASA Image and Video Library

    2017-12-08

    "Light Echo" Illuminates Dust Around Supergiant Star V838 Monocerotis (V838 Mon) Credit: NASA and The Hubble Heritage Team (AURA/STScI) The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. Goddard is responsible for HST project management, including mission and science operations, servicing missions, and all associated development activities. To learn more about the Hubble Space Telescope go here: www.nasa.gov/mission_pages/hubble/main/index.html NASA Goddard Space Flight Center is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. Follow us on Twitter Join us on Facebook

  20. Finding our Origins with the Hubble and James Webb Space Telescopes

    NASA Technical Reports Server (NTRS)

    Gardner, Jonathan

    2008-01-01

    NASA is planning a successor to the Hubble Space Telescope designed to study the origins of galaxies, stars, planets and life in the universe. In this talk, Dr. Gardner will discuss the origin and evolution of galaxies, beginning with the Big Bang and tracing what we have learned with Hubble through to the present day. He will show that results from studies with Hubble have led to plans for its successor, the James Webb Space Telescope. Webb is scheduled to launch in 2013, and is designed to find the first galaxies that formed in the distant past and to penetrate the dusty clouds of gas where stars are still forming today. He will compare Webb to Hubble, and discuss recent progress in the construction of the observatory.

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