UBVRI Systems: Resolving Different Versions

Details UBVRI Systems: Resolving Different Versions UBVRI Systems: Resolving Different Versions

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasp..107..672b&link_type=abstract

Publications of the Astronomical Society of the Pacific, v.107, p.672

Astronomy and Astrophysics

Astronomy

38

Methods: Numerical, Stars: Fundamental Parameters

Scientific paper

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. (SECTION: Stars)

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