M31 Long Period Variables : Photometry (Mould+, 2004)

Details M31 Long Period Variables : Photometry (Mould+, 2004) M31 Long Period Variables : Photometry (Mould+, 2004)

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..21540623m&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/154/623. Originally published in: 2004ApJS..154..623M

Physics

Stars: Variable, Photometry: Cousins, Photometry: Infrared

Scientific paper

The observations upon which this paper is based were taken over a period of more than 6yr from Palomar Observatory. We surveyed 64 fields in M31 with the 60inch telescope, equipped with a refractive reimager including an f/1.2 camera and a TI 800x800 CCD. The pixel scale was approximately 0.6"/pixel and exposure times were 5minutes per field, to avoid saturation of the brightest LPVs. All observations were made in the I band, usually close to full moon.
(1 data file).

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