Segmentation maps from degraded HST image
Until now, the segmentation maps were created from the original resolution HST image, then warped to the grid of MUSE. However, the mixed pixels that were created would bias the position measurements of the objects, so now, we are using NoiseChisel on the degraded HST image. But since there is practically no noise left in those images, we use very lax NoiseChisel parameters. Also, the Sky value of the HST images is subtracted before convolution.
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