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8 papers · 2 filters
The large and small scale properties of the intergalactic gas in the Slug Ly-alpha nebula revealed by MUSE HeII emission observations
Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly +11
With a projected size of about 450 kpc at z~2.3, the Slug Ly-alpha nebula is a rare laboratory to study, in emission, the properties of the intergalactic gas in the Cosmic Web. Sin…
The MUSE-Wide Survey: A determination of the Lyman emitter luminosity function at
Edmund Christian Herenz, Lutz Wisotzki, Rikke Saust +11
(Abridged) We investigate the Lyman emitter luminosity function (LAE LF) within the redshift range from the first instalment of the blind integral field spe…
The MUSE-Wide Survey: Survey Description and First Data Release
T. Urrutia, L. Wisotzki, J. Kerutt +17
We present the MUSE-Wide survey, a blind, 3D spectroscopic survey in the CANDELS/GOODS-S and CANDELS/COSMOS regions. Each MUSE-Wide pointing has a depth of 1 hour and hence targets…
The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last 10 Gyr
Alfred L. Tiley, A. M. Swinbank, C. M. Harrison +16
We analyse maps of the spatially-resolved nebular emission of 1500 star-forming galaxies at - from deep KMOS and MUSE observations to measure the average…
MUSE Spectroscopic Identifications of Ultra-Faint Emission Line Galaxies with M -15
Michael V. Maseda, Roland Bacon, Marijn Franx +16
Using an ultra-deep blind survey with the MUSE integral field spectrograph on the ESO Very Large Telescope, we obtain spectroscopic redshifts to a depth never explored before: gala…
The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at
Leindert A. Boogaard, Jarle Brinchmann, Nicolas Bouché +16
Star-forming galaxies have been found to follow a relatively tight relation between stellar mass () and star formation rate (SFR), dubbed the `star formation sequence'. A tu…
MUSE crowded field 3D spectroscopy in NGC300 I. First results from central fields
M. M. Roth, C. Sandin, S. Kamann +9
Aims. As a new approach to the study of resolved stellar populations in nearby galaxies, our goal is to demonstrate in NGC300 that integral field spectroscopy with high spatial res…
The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
Anna Feltre, Roland Bacon, Laurence Tresse +18
The physical origin of the near-ultraviolet MgII emission remains an under-explored domain, contrary to more typical emission lines detected in the spectra of star-forming galaxies…