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more examples of problematic galaxy modeling #454
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From Peter:
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I spot-checked several of these and I don't think there are any specific action items. Galaxies that are large enough to be in the LSLGA (see #536 and #513) will get pre-burned and will have non-parametric ellipse-fitting quantities measured. Galaxies too small to be in the LSLGA but large enough to have their internal / spiral structure will get More complex galaxy modeling will need to be done outside of the scope of the main data releases. |
Problem areas identified by Maayane Soumagnac (working with Peter Nugent).
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