Expanding the Standard Star Library Using CCD Photometry

Details Expanding the Standard Star Library Using CCD Photometry Expanding the Standard Star Library Using CCD Photometry

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.7605a&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #76.05; Bulletin of the American Astronomical Society, Vol. 34, p.1226

Astronomy and Astrophysics

Astronomy

Scientific paper

Taylor and Joner (1996) showed consistency between PM photometry standard fields observered by Landolt (1983,1992), Graham (1983), and Cousins (1974). CCD data from subsections of standard equatorial fields using VRI filters were secured by Joner from 1993 to 1995 at CTIO. Six fields, SA98, SA102, SA106, SA110, SA114, and an asterism in M67 are being analyzed using aperture phtometry techniques. The ultimate goal is to expand the number of standard stars in the current standard fields to include fainter stars. Results of this analysis will be presented.

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