Improved u'g'r'i'z' to UBVRCIC Transformation Equations for Main Sequence Stars
Abstract
We report improved transformation equations between the u'g'r'i'z' and UBVRCIC photometric systems. Although the details of the transformations depend on luminosity class, we find a typical rms scatter on the order of 0.001 magnitude if the sample is limited to main sequence stars. Furthermore, we find an accurate transformation requires complex, multi-color dependencies for the bluer bandpasses. Results for giant stars will be reported in a subsequent paper.
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