activity
20172020
most citedThe MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

180 citations · 348 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202048 cited

AstroSat detection of Lyman continuum emission from a z=1.42 galaxy

Kanak Saha, Shyam N. Tandon, Charlotte Simmonds +10

One of the outstanding problems of current observational cosmology is to understand the nature of sources that produced the bulk of the ionizing radiation after the Cosmic Dark Age…

astro-ph.GA201911 cited

Spatially resolved signature of quenching in star-forming galaxies

Salvatore Quai, Lucia Pozzetti, Michele Moresco +5

Understanding when, how and where star formation ceased (quenching) within galaxies is still a critical subject in galaxy evolution studies. Taking advantage of the new methodology…

astro-ph.GA201960 cited

Exploring HeII1640 emission line properties at

Themiya Nanayakkara, Jarle Brinchmann, Leindert Boogaard +10

Deep optical spectroscopic surveys of galaxies provide us a unique opportunity to investigate rest-frame ultra-violet (UV) emission line properties of galaxies at .…

astro-ph.GA2018

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…

astro-ph.GA2018

Properties and redshift evolution of star-forming galaxies with high [OIII]/[OII] ratios with MUSE at 0.28<z<0.85

M. Paalvast, A. Verhamme, L. A. Straka +21

We present a study of the [OIII]5007/[OII]3727 (O32) ratios of star-forming galaxies drawn from MUSE data spanning a redshift range 0.28<z<0.85. Recently discovered Lyman continuum…

astro-ph.GA201737 cited

The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies

Hayley Finley, Nicolas Bouché, Thierry Contini +15

Non-resonant FeII* 2365, 2396, 2612, 2626 emission can potentially trace galactic winds in emission and provide useful constraints to wind models. From the 3'x3' mosaic of the Hubb…