Photometric Stability of the NURO Photometrics CCD

Details Photometric Stability of the NURO Photometrics CCD Photometric Stability of the NURO Photometrics CCD

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...18110109l&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #101.09; Bulletin of the American Astronomical Society, Vol. 24, p.1282

Astronomy and Astrophysics

Astronomy

Scientific paper

During four completely clear nights in September 1992, we observed a number of Landolt standard stars using the Lowell 31 inch telescope, located on Anderson Mesa near Flagstaff, and the National Undergraduate Research Observatory (NURO) CCD system. The CCD system uses a TEK 512 back-illuminated, metachrome coated chip. We used BVRI filters. We will report on the repeatability of the standard star measurements, on both hourly and night to night time scales, and on the accuracy and repeatability of the transformation from our filter system to the standard BVRI system.

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