The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5

We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ≈150 h on-source of integral field optical spectroscopy in a 1.5 ...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2019-11, Vol.490 (1), p.1451-1469
Hauptverfasser: Fossati, M, Fumagalli, M, Lofthouse, E K, D’Odorico, V, Lusso, E, Cantalupo, S, Cooke, R J, Cristiani, S, Haardt, F, Morris, S L, Peroux, C, Prichard, L J, Rafelski, M, Smail, I, Theuns, T
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Sprache:eng
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