Spectroscopy and Imaging of the MUSE Ultra Deep Field (MUDF)

The MUSE Ultra Deep Field is a unique region of the sky hosting two physically-associated quasars that allow us to study the connections between galaxies and their surrounding gas using emission and absorption line spectroscopy. Using HST observations of this field, we have created custom-calibrated data products that include the following: WFC3 F140W, F125W, and F336W mosaics; 1D and 2D WFC3 G141 grism spectra, and re-calibrated archival WFPC2 F702W and F450W mosaics. We have also generated source catalogs using Source Extractor, and measured galaxy morphologies using Statmorph. We plan to provide all of the science images, point spread function models, extracted grism spectra, and source catalogs as HLSPs that can be used by the community for a variety of investigations. In the future, we plan to expand the collection to include additional data products.