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Proceedings Paper

Phase-referenced imaging and micro-arcsecond astrometry with the VLTI
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Paper Abstract

An update of the current status and schedule of PRIMA (Phase-Referenced Imaging and Micro-arcsecond Astrometry) developed for the Very Large Telescope Interferometer (VLTI) is given, with emphasis on the astrometric objectives, performances and technological challenges. PRIMA will allow to observe simultaneously two fields separated by 2 to 60 arcsec, to detect and track the fringes on the brightest object, to detect the fringes on the faintest, and to measure the phase of the secondary set of fringes relative to the primary one, with an accuracy of (lambda) /1000 at 2 micrometers .

Paper Details

Date Published: 5 July 2000
PDF: 12 pages
Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); doi: 10.1117/12.390229
Show Author Affiliations
Francoise Delplancke, European Southern Observatory (Belgium)
Samuel A. Leveque, European Southern Observatory (Germany)
Pierre Kervella, European Southern Observatory (Germany)
Andreas Glindemann, European Southern Observatory (Germany)
Luigi D'Arcio, Space Research Organization Netherlands (Netherlands)


Published in SPIE Proceedings Vol. 4006:
Interferometry in Optical Astronomy
Pierre J. Lena; Andreas Quirrenbach, Editor(s)

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