110 citations · 341 across the 8 of their papers we have counts for
8 papers
The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
Anna Feltre, Michael V. Maseda, Roland Bacon +22
We investigate the ultraviolet (UV) spectral properties of faint Lyman- emitters (LAEs) in the redshift range 2.9<z<4.6 and provide material to prepare future observations of th…
An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
Ivana Barišić, Arjen van der Wel, Josha van Houdt +7
Maintenance-mode feedback from low-accretion rate AGN, manifesting itself observationally through radio-loudness, is invoked in all cosmological galaxy formation models as a mechan…
Does radiative feedback make faint z>6 galaxies look small?
Sylvia Ploeckinger, Joop Schaye, Alvaro Hacar +3
Recent observations of lensed sources have shown that the faintest () galaxies observed at z=6-8 appear to be extremely compact. Some of…
The MUSE Atlas of Disks (MAD): Resolving Star Formation Rates and Gas Metallicities on < 100pc Scales
Santiago Erroz-Ferrer, C. Marcella Carollo, Mark den Brok +13
We study the physical properties of the ionized gas in local disks using the sample of 38 nearby M Star-Forming Main Sequence (SFMS) galaxies observed so…
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…
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot +14
Interpreting observations of distant galaxies in terms of constraints on physical parameters - such as stellar mass, star-formation rate (SFR) and dust optical depth - requires spe…