A study of the photometric systems of the CdC and AGK catalogs and their derivatives

Details A study of the photometric systems of the CdC and AGK catalogs and their derivatives A study of the photometric systems of the CdC and AGK catalogs and their derivatives

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...65p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 2, Mar.-Apr. 1992, p. 65-70. In Russian.

Astronomy and Astrophysics

Astronomy

Astrometry, Astronomical Catalogs, Stellar Luminosity, Stellar Spectrophotometry, Error Analysis, Least Squares Method, Sky Surveys (Astronomy), Stellar Magnitude

Scientific paper

Systematic (up to 0.5-1 m) and random (up to +/-0.5 m) errors in brightness estimates for stars in the CdC and AGK catalogs are determined through a comparison with photoelectric stellar magnitudes in the B system. When using stellar magnitudes from these catalogs, the magnitude values should be adjusted for the scaling and zero-point errors, and a conversion should be made from star image diameters (CdC or m(pg) (AGK) to B magnitudes.

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