The impact of satellite trails on Hubble Space Telescope observations
The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
The MUSE Ultra Deep Field (MUDF). IV. A pair of X-ray weak quasars at the heart of two extended Lya nebulae
The MUSE Ultra Deep Field (MUDF). V. Characterizing the Mass-Metallicity Relation for Low-mass Galaxies at z ~ 1-2
Instrument
WFC3/UVIS
Temporal Coverage
2020-05-05T16:44:25Z/2020-07-12T20:25:53Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Fossati et al., 2020, 'Paths to quiescence: gaseous feeding, morphology and star-formation histories of galaxies from the HST+MUSE Ultra Deep Field', 1.0, European Space Agency, https://doi.org/10.5270/esa-191zhb3