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The origin of UV emission in extremely low-mass satellite galaxies: Insights from Leo T
S Amrutha, Mousumi Das, Daniel Vaz +1
Leo T, a Milky Way (MW) satellite, is the lowest-mass gas-rich galaxy known to show recent star formation, making it an excellent laboratory for investigating star formation in the…
Are High-EW LAEs good analogs for the earliest galaxies? A study on the ionizing conditions and gas properties of LAEs at $2\lesssim z\lesssim7
Lena Pless, Themiya Nanayakkara, Karl Glazebrook +3
Lyman- emitters (LAEs) are frequently proposed as analogs of the low-mass, metal-poor galaxies thought to dominate cosmic reionization. In particular, galaxies with large Ly…
The MUSE-Faint survey. IV. Dissecting Leo T, a gas-rich relic with recent star formation
Daniel Vaz, Jarle Brinchmann, Sebastiaan L. Zoutendijk +6
Leo T () is both the faintest and the least massive galaxy known to contain neutral gas and to display signs of recent star formation. We analyse photometry and stellar…
The Tully-Fisher relation in dense groups at in the MAGIC survey
Valentina Abril-Melgarejo, Benoît Epinat, Wilfried Mercier +11
Galaxies in dense environments are subject to interactions and mechanisms which directly affect their evolution by lowering their gas fractions and reducing their star-forming capa…
The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
J. Brinchmann, H. Inami, R. Bacon +14
We tested the performance of photometric redshifts for galaxies in the Hubble Ultra Deep field down to 30th magnitude. We compared photometric redshift estimates from three spectra…
The MUSE-Wide Survey: A first catalogue of 831 emission line galaxies
E. C. Herenz, T. Urrutia, L. Wisotzki +11
We present a first instalment of the MUSE-Wide survey, covering an area of 22.2 arcmin (corresponding to 20% of the final survey) in the CANDELS/Deep area of the Chandra…
A young star-forming galaxy at z = 3.5 with an extended Ly\, halo seen with MUSE
Vera Patrício, Johan Richard, Anne Verhamme +12
Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We pre…