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High-accuracy propagation of light rays

Published online by Cambridge University Press:  06 January 2010

Pierre Teyssandier
Pierre Teyssandier*
Affiliation:
Dépt SYstèmes de Référence Temps-Espace (SYRTE), CNRS-UMR 8630 & UPMC, Observatoire de Paris, 61 avenue de l'Observatoire, 75014 Paris email: Pierre.Teyssandier@obspm.fr
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Abstract

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We present a review of the different methods currently developed to determine the deflection of light rays due to gravity. The aim of these methods is primarily to calculate the angular distances with an accuracy of the order of microarcsecond.

Keywords

Gravitationastrometryreference systems
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. 103 - 111
Copyright
Copyright © International Astronomical Union 2010

References

Brumberg, V. A. 1987, Kinematics Phys. Celest. Bodies, 3, 6Google Scholar
Brumberg, V. A. 1991, Essential Relativistic Celestial Mechanics (Bristol: Adam Hilger), p. 200Google Scholar
Crosta, M. T. & Mignard, F. 2006, Class. Quantum Grav., 23, 4853CrossRefGoogle Scholar
de Felice, F., Vecchiato, A., Crosta, M. T., Bucciarelli, B., & Lattanzi, M. G. 2006, ApJ, 653, 1552CrossRefGoogle Scholar
de Jans, C. 1922, Mém. Acad. Roy. Belgique Cl. Sci., 6, pp. 1–26; 6, pp. 27–41Google Scholar
Klioner, S. A. & Kopeikin, S. M. 1992, Astron. J., 104, 897CrossRefGoogle Scholar
Klioner, S. A. & Soffel, M. H. 2000, Phys. Rev. D, 62, 024019CrossRefGoogle Scholar
Klioner, S. A. 2003, Astron. J., 125, 1580CrossRefGoogle Scholar
Klioner, S. A & Soffel, M. H. 2004, in: Turon, C., O'Flaherty, K. S., & Perryman, M. A. C. (eds.), Proceedings of the Symposium “The Three-Dimensional Universe with Gaia” (ESA SP-576, 2005), p. 305Google Scholar
Kopeikin, S. M. 1997, J. Math. Phys., 38, 2587CrossRefGoogle Scholar
Kopeikin, S. M. & Schäfer, G. 1999, Phys. Rev. D, 60, 124002CrossRefGoogle Scholar
Kopeikin, S. M., Korobkov, P., & Polnarev, A. 2006, Class. Quantum Gravity, 23, 4299CrossRefGoogle Scholar
Kopeikin, S. M. & Makarov, V. V. 2007, Phys. Rev. D, 75, 062002CrossRefGoogle Scholar
Le Poncin-Lafitte, C., Linet, B., & Teyssandier, P. 2004, Class. Quantum Gravity, 21, 4463CrossRefGoogle Scholar
Le Poncin-Lafitte, C., & Teyssandier, P. 2008, Phys. Rev. D, 77, 044029CrossRefGoogle Scholar
Minazzoli, O., & Chauvineau, B. 2009, Phys. Rev. D, 79, 084027CrossRefGoogle Scholar
Soffel, M. H. 1989, Relativity in Astrometry, Celestial Mechanics and Geodesy (Berlin: Springer-Verlag)CrossRefGoogle Scholar
Teyssandier, P., & Le Poncin-Lafitte, C. 2006, arXiv:gr-qc/0611078Google Scholar
Teyssandier, P., & Le Poncin-Lafitte, C. 2008, Class. Quantum Gravity, 25, 145020CrossRefGoogle Scholar
Will, C. M. 1988, Am. J. Phys., 56, 413CrossRefGoogle Scholar
Zschocke, S. & Klioner, S. A. 2009, arXiv:astro-ph/09043704Google Scholar