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

MPS-Authors
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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;

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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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Citation

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: http://hdl.handle.net/11858/00-001M-0000-0023-F9DB-D
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