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Sample records for lauksaimniecbas universittes aentra

  1. Webis at TREC 2014: Web, Session, and Contextual Suggestion Tracks

    DTIC Science & Technology

    2014-11-01

    Webis at TREC 2014: Web, Session, and Contextual Suggestion Tracks Matthias Hagen Steve Göring Maximilian Michel Georg Müller Benno Stein Bauhaus ...ES) Bauhaus -Universit??t Weimar,99421 Weimar, Germany, 8. PERFORMING ORGANIZATION REPORT NUMBER 9. SPONSORING/MONITORING AGENCY NAME(S) AND ADDRESS

  2. Wave Modelling - The State of the Art

    DTIC Science & Technology

    2007-09-27

    Heverlee, Belgium q Universitt) di Torino, Dipartimento di Fisica Generale, Via P. Giuria 1, 10125 Torino, Italy A. M. Obukhov Institute for Physics of... molecular processes. Van Duin and Janssen (1992) pointed out that this approach fails for low-frequency waves. Mixing length modelling assumes that

  3. Monetary and Fiscal Policy Interactions in the Euro Area

    DTIC Science & Technology

    2004-03-01

    Helmut-Schmidt-Universitft Universit~t der Bundeswehr Hamburg University of the Federal Armed Forces Hamburg ,Fchergruppe Volkswirtschaftslehre ...Output 985 1015 Change in Government Purchases 10 - 10 Output 1000 1000 Bisher erschienen: Diskussionspapiere der Fichergruppe Volkswirtschaftslehre ...Theoretische Volkswirtschaftslehre * Brauninger, Michael, Social Capital and Regional Mobility, Nr. 4/2002. * SchMfer, Wolf, EU-Erweiterung: Anmerkungen zum

  4. HiFi-MBQC High Fidelitiy Measurement-Based Quantum Computing using Superconducting Detectors

    DTIC Science & Technology

    2016-04-04

    computer. We exploit the conceptual framework of measurement - based quantum computation that enables a client to delegate a computation to a quantum...AFRL-AFOSR-UK-TR-2016-0006 HiFi-MBQC High Fidelitiy Measurement - Based Quantum Computing using Superconducting Detectors Philip Walther UNIVERSITT...HiFi-MBQC High Fidelitiy Measurement - Based Quantum Computing using Superconducting Detectors 5a. CONTRACT NUMBER FA8655-11-1-3004 5b. GRANT NUMBER

  5. The Mass of the Candidate Exoplanet Companion to HD 136118 from Hubble Space Telescope Astrometry and High-Precision Radial Velocities

    NASA Astrophysics Data System (ADS)

    Martioli, Eder; McArthur, Barbara E.; Benedict, G. Fritz; Bean, Jacob L.; Harrison, Thomas E.; Armstrong, Amber

    2010-01-01

    We use Hubble Space Telescope fine guidance sensor astrometry and high-cadence radial velocities for HD 136118 from the Hobby-Eberly Telescope with archival data from Lick to determine the complete set of orbital parameters for HD 136118 b. We find an orbital inclination for the candidate exoplanet of ib = 163fdg1 ± 3fdg0. This establishes the actual mass of the object, Mb = 42+11 -18 MJ , in contrast to the minimum mass determined from the radial velocity data only, Mb sin i ~ 12 MJ . Therefore, the low-mass companion to HD 136118 is now identified as a likely brown dwarf residing in the "brown dwarf desert." 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 NAS5-26555. Based on observations obtained with the Hobby-Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Stanford University, Ludwig-Maximilians-Universitt München, and Georg-August-Universität Göttingen.

  6. New Observational Constraints on the υ Andromedae System with Data from the Hubble Space Telescope and Hobby-Eberly Telescope

    NASA Astrophysics Data System (ADS)

    McArthur, Barbara E.; Benedict, G. Fritz; Barnes, Rory; Martioli, Eder; Korzennik, Sylvain; Nelan, Ed; Butler, R. Paul

    2010-06-01

    We have used high-cadence radial velocity (RV) measurements from the Hobby-Eberly Telescope with existing velocities from the Lick, Elodie, Harlan J. Smith, and Whipple 60'' telescopes combined with astrometric data from the Hubble Space Telescope Fine Guidance Sensors to refine the orbital parameters and determine the orbital inclinations and position angles of the ascending node of components υ And A c and d. With these inclinations and using M * = 1.31M sun as a primary mass, we determine the actual masses of two of the companions: υ And A c is 13.98+2.3 -5.3 M JUP, and υ And A d is 10.25+0.7 -3.3 M JUP. These measurements represent the first astrometric determination of mutual inclination between objects in an extrasolar planetary system, which we find to be 29fdg9 ± 1°. The combined RV measurements also reveal a long-period trend indicating a fourth planet in the system. We investigate the dynamic stability of this system and analyze regions of stability, which suggest a probable mass of υ And A b. Finally, our parallaxes confirm that υ And B is a stellar companion of υ And A. 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 NAS5-26555. Based on observations obtained with the Hobby-Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Stanford University, Ludwig-Maximilians-Universitt Mnchen, and Georg-August-Universität Göttingen.