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MusE GAs Flow and Wind (MEGAFLOW) VI. A study of CIV and MgII absorbing gas surrounding [OII] emitting galaxies
Ilane Schroetter, Nicolas F. Bouché, Johannes Zabl +7
Using the MEGAFLOW survey, which consists of a combination of MUSE and UVES observations of 22 quasar fields selected to contain strong MgII absorbers, we measure covering fraction…
High-resolution imaging follow-up of doubly imaged quasars
Anowar J. Shajib, Eden Molina, Adriano Agnello +8
We report upon three years of follow-up and confirmation of doubly imaged quasar lenses through imaging campaigns from 2016-2018 with the Near-Infrared Camera2 (NIRC2) on the W. M.…
Revealing the Impact of Quasar Luminosity on Giant Ly Nebulae
Ruari Mackenzie, Gabriele Pezzulli, Sebastiano Cantalupo +6
We present the results from a MUSE survey of twelve quasars, which were selected to be much fainter (20<i<23) than in previous studies of Giant Ly Nebulae around t…
Spatially resolved CIII]1909 emission in Haro 11
Genoveva Micheva, Göran Östlin, Jens Melinder +7
The CIII]1909 (hereafter, C III]) line is the strongest ultraviolet emission line after Ly and is therefore of interest to high redshift studies of star-forming (SF) galaxies ne…
The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at with CO stacking of MUSE detected Galaxies
Hanae Inami, Roberto Decarli, Fabian Walter +19
We report molecular gas mass estimates obtained from a stacking analysis of CO line emission in the ALMA Spectroscopic Survey (ASPECS) using the spectroscopic redshifts from the op…
An Atlas of MUSE Observations towards Twelve Massive Lensing Clusters
Johan Richard, Adélaïde Claeyssens, David J. Lagattuta +25
Spectroscopic surveys of massive galaxy clusters reveal the properties of faint background galaxies, thanks to the magnification provided by strong gravitational lensing. We presen…
The nature of CR7 revealed with MUSE: a young starburst powering extended Lyman- emission at z=6.6
Jorryt Matthee, Gabriele Pezzulli, Ruari Mackenzie +11
CR7 is among the most luminous Lyman- emitters (LAEs) known at and consists of at least three UV components that are surrounded by Lyman- (Ly) emission. Previous…
Circumnuclear Molecular Gas in Low-redshift Quasars and Matched Star-forming Galaxies
Takuma Izumi, John D. Silverman, Knud Jahnke +6
A series of gravitational instabilities in a circumnuclear gas disk (CND) are required to trigger gas transport to a central supermassive black hole (SMBH) and ignite Active Galact…
The Data Processing Pipeline for the MUSE Instrument
Peter M. Weilbacher, Ralf Palsa, Ole Streicher +12
Processing of raw data from modern astronomical instruments is nowadays often carried out using dedicated software, so-called "pipelines" which are largely run in automated operati…
Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
Michael V. Maseda, Roland Bacon, Daniel Lam +16
While low-luminosity galaxies dominate number counts at all redshifts, their contribution to cosmic Reionization is poorly understood due to a lack of knowledge of their physical p…
The MUSE Hubble Ultra Deep Field Survey XIII. Spatially resolved spectral properties of Lyman alpha haloes around star-forming galaxies at z > 3
Floriane Leclercq, Roland Bacon, Anne Verhamme +18
We present spatially resolved maps of six individually-detected Lyman alpha haloes (LAHs) as well as a first statistical analysis of the Lyman alpha (Lya) spectral signature in the…