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/IR
Temporal Coverage
2019-08-10T13:55:32Z/2020-09-09T12:06:38Z
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, Rafelski comma Marc, 2020, 'Exploring the gaseous surroundings of low-mass galaxies with an HST+MUSE Deep Field', 1.0, European Space Agency, https://doi.org/10.5270/esa-w2lvb99