Improved ugriz to UBV RCIC Transformation Equations for Main Sequence Stars


We report improved transformation equations between the ugriz and UBV RCIC 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… (More)


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