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Mohammad Akhlaghi authored
The MUSE PSFs were given as parameters to a Moffat function fit. So they were created using Gnuastro's MakeProfiles. The HST PSF was also generated from one of the bright stars in the UDF. It isn't the brightest, but so far we haven't checked if it was saturated or not. However, apparently, Gnuastro's convolve had problems in finding the kernel to convolve with the HST image to get to the MUSE resolution. So for now, we have kept the rules (to work on them later), but they are currently ignored in the pipeline (they aren't a prerequisite to anything). Since the MUSE PSF is much wider than the HST, for now, we will just convolve the HST image with the MUSE PSF. Later, when the problem above is solved, we will find the proper kernel more accurately.
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