Reaching micro-arcsecond astrometry with long baseline optical interferometry - 
application to the GRAVITY instrument

Lacour, S.; Eisenhauer, F.; Gillessen, S.; Pfuhl, O.; Woillez, J.; Bonnet, H.; Perrin, G.; Lazareff, B.; Rabien, S.; Lapeyrère, V.; Clénet, Y.; Kervella, P.; Kok, Y.

doi:10.1051/0004-6361/201423940

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Reaching micro-arcsecond astrometry with long baseline optical interferometry - application to the GRAVITY instrument

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Eisenhauer, F.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Gillessen, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Pfuhl, O.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4786

Rabien, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Kok, Y.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lacour, S., Eisenhauer, F., Gillessen, S., Pfuhl, O., Woillez, J., Bonnet, H., et al. (2014). Reaching micro-arcsecond astrometry with long baseline optical interferometry - application to the GRAVITY instrument. Astronomy & Astrophysics, 567: A75. doi:10.1051/0004-6361/201423940.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0023-F9DB-D

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