Add documentation of qfit/cfit relation to chi and sharp #2143
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This is a code-wise trivial but conceptually important clarification that qfit and cfit are similar to "chi" and "sharp" as used in DAOPHOT. Of course it already mentions the hst1pass connection, but a lot of people I know who do crowded field stellar photometry are more familiar with the DAOPHOT and DOLPHOT terminology, so it seems useful to add that connection as well.