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Mohammad Akhlaghi authored
Until now NoiseChisel was ran on the HST images and the segmentation map was used for the comparisons of both magitude and astrometry. While this is accurate for the former, it is not so good for the latter, especially as the targets become fainter. The shape of the segmentation map (from HST) will bias the shallower MUSE astrometry. So for astrometry, we done the opposite: doing detection on MUSE and using its segmentation map on both MUSE and HST. The final comparison catalogs are now made with this commit and we can go onto the statistics.
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