Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-24T17:20:58.218Z Has data issue: false hasContentIssue false
  • English
  • Français

Gaia: Relativistic modelling and testing

Published online by Cambridge University Press:  06 January 2010

F. Mignard  and
S. A. Klioner
F. Mignard
Affiliation:
Observatoire de la Côte d'Azur, Nice, France email: [email protected]
S. A. Klioner
Affiliation:
Lohrmann Observatory, Dresden Technical University, Dresden, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Gaia is an ambitious space astrometry mission of ESA with a main objective to map the sky in astrometry and photometry down to a magnitude 20 by the end of the next decade. Given its extreme astrometric accuracy and the repeated observations over five years, the observation modelling is done in a fully relativistic framework and several tests of General Relativity or of its extensions can be carried out during the data processing. The paper presents an overview of the current activities in this area and of the expected performances.

Keywords

astrometryrelativitydata processing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S261: Relativity in Fundamental Astronomy: Dynamics, Reference Frames, and Data Analysis , April 2009 , pp. 306 - 314
Copyright
Copyright © International Astronomical Union 2010

References

Anglada Escudé, G., Klioner, S., & Torra, J., 2007, Relativistic light deflection near giant planets using gaia astrometry, in MG11 Proceedings., Kleinert, H. & Jantzen, R. T. eds., p. 2588.Google Scholar
Bertotti, B., Iess, L., & Tortora, P., 2003, Nature 425, 374.Google Scholar
de Bruijne, J., 2010, this proceedings, 331CrossRefGoogle Scholar
Crosta, M. T. & Mignard, F., 2006, Classical and Quantum Gravity 23, 4853.CrossRefGoogle Scholar
Damour, T. & Nordtvedt, K., 1993, Phys. Rev. Lett. 70, 2217.Google Scholar
Damour, T. & Nordtvedt, K., 1993, Phys. Rev. D 48, 3436.CrossRefGoogle Scholar
Froeschlé, M., Mignard, F. , F., & Arenou, F., 1997, Determination of the PPN parameter γ with the Hipparcos data, in Proceedings of the ESA Symposium “Hipparcos – Venice 97”, ESA SP-402.Google Scholar
Fuchs, B. & Bastian, U., 2005, Weighing stellarmass black holes with gaia, in ESA SP-576: The Three-Dimensional Universe with Gaia, eds. Turon, C., O'Flaherty, K. S. and Perryman, M. A. C..Google Scholar
Gwinn, C., Eubanks, T., Pyne, T., Birkinshaw, M., & Matsakis, D., 1997, Astrophys. J. 485, 87.CrossRefGoogle Scholar
Hestroffer, D., et al. , 2007, Relativistic tests from the motion of the asteroids, in MG11 Proceedings., Kleinert, H. & Jantzen, R. T. eds., p. 2600.CrossRefGoogle Scholar
Hestroffer, D., Mouret, S., Mignard, F., Tanga, P., & Berthier, J. 2010, this proceedings, 325Google Scholar
Hobbs, D., Holl, B., Lindegren, L., Raison, F., Klioner, S., & Butkevich, A., 2010, this proceedings, 315Google Scholar
Klioner, S. A., 2003, AJ 125, 1580.CrossRefGoogle Scholar
Laemmerzahl, C., 2006, Test theories for Lorentz invariance, in Lect. Notes Physics, Springer, 702, 349.CrossRefGoogle Scholar
Mansouri, R. & Sexl, R., 1977, Gen. Rel. Grav. 8, p. 497.CrossRefGoogle Scholar
Mignard, F. & Klioner, S., 2007, Space Astrometry and Relativity, in MG11 Proceedings., Kleinert, H. & Jantzen, R. T. eds., p. 245.Google Scholar
Pyne, T., Gwinn, C., Birkinshaw, M., Eubanks, T., & Matsakis, D., 1996, Astrophys. J. 465, 566.Google Scholar
Robertson, H., 1949, Rev. Mod. Phys. 21, 378.CrossRefGoogle Scholar