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Currently stars with bad photometry (any magnitude/color with values outside the range [-50., 50.]) are discarded before the center, RDP and radius are obtained.
These stars can help with a better determination of the cluster's structure and should be discarded after this initial functions are appliednot be discarded, but masked.
Currently stars with bad photometry (any magnitude/color with values outside the range [-50., 50.]) are discarded before the center, RDP and radius are obtained.
These stars can help with a better determination of the cluster's structure and should
be discarded after this initial functions are appliednot be discarded, but masked.Related: #14, #68.
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