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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…
Galaxy and Quasar Fueling Caught in the Act from the Intragroup to the Interstellar Medium
Sean D. Johnson, Hsiao-Wen Chen, Lorrie A. Straka +11
We report the discovery of six spatially extended (10-100 kpc) line-emitting nebulae in the z=0.57 galaxy group hosting PKS0405-123, one of the most luminous quasars at z<1. The di…
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…
Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies
L. Wisotzki, R. Bacon, J. Brinchmann +22
Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurement…
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…