MAD observations of {sigma} Ori (Bouy+, 2009)

Details MAD observations of {sigma} Ori (Bouy+, 2009) MAD observations of {sigma} Ori (Bouy+, 2009)

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..34930931b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/493/931. Originally published in: 2009A&A...493..931B

Physics

Associations: Stellar, Stars: Nearby, Photometry: Infrared

Scientific paper

MAD is a prototype instrument performing wide field-of-view, real-time correction for atmospheric turbulence. MAD was built by the European Southern Observatory (ESO) with the contribution of two external consortia to prove the feasibility of MCAO on the sky in the framework of the 2nd generation VLT instrumentation and of the European Extremely Large Telescope. During the on-sky demonstration run of MAD held in November 2007, a region of 1.5'x1.5' centered on the sigma-Orionis cluster was observed in the H and Ks filters.
(2 data files).

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