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UBVRI SYSTEMS: RESOLVING DIFFERENT VERSIONS

© 1995. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
, , Citation Michael S. Bessell 1995 PASP 107 672 DOI 10.1086/133607

1538-3873/107/713/672

ABSTRACT

The photometry of Landolt has been transformed onto the Cousins (SAAO) system by using polynomial fits to photometry of 230 common stars. The accuracy of the fits are within 0.01 mag for (B-V), (R-I), and (V-I) and 0.02 mag for (U-B). The BVRI photometry of Bessell and Weis has also been transformed.

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10.1086/133607