Astra: Dual-field And Astrometry With The Keck Interferometer

Details Astra: Dual-field And Astrometry With The Keck Interferometer Astra: Dual-field And Astrometry With The Keck Interferometer

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21743315w&link_type=abstract

American Astronomical Society, AAS Meeting #217, #433.15; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astrophysics

Scientific paper

Funded in 2006 by an NSF MRI grant, the ASTRA project aims at improving the capability of the Keck interferometer by providing a spectro-interferometric mode for R 2000 spectroscopy in the K band, a phase referencing mode to reach K 14 magnitude, and an astrometric mode for 100-30 micro-arcsecond narrow angle astrometry. These improvements cover a broad range of astrophysical topics including Young Stellar Objects, Active Galactic Nuclei, the Galactic Center, and known Exo-planets.

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