220 citations · 571 across the 9 of their papers we have counts for
22 papers
On the relation between Lya absorbers and local galaxy filaments
Sietske J. D. Bouma, Philipp Richter, Martin Wendt
The intergalactic medium (IGM) is believed to contain the majority of baryons in the universe and to trace the same dark matter structure as galaxies, forming filaments and sheets.…
Mapping the youngest and most massive stars in the Tarantula nebula with MUSE-NFM
N. Castro, M. M. Roth, P. M. Weilbacher +7
The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are the key to provide anchors to calibrate theory, however performing these stud…
MusE GAs FLOw and Wind (MEGAFLOW) V. The dust/metallicity-anisotropy of the Circum-Galactic Medium
Martin Wendt, Nicolas F. Bouché, Johannes Zabl +2
We investigate whether the dust content of the circum-galactic medium (CGM) depends on the location of the quasar sightline with respect to the galaxy major-axis using 13 galaxy-Mg…
A stellar census in globular clusters with MUSE -- Extending the CaT-metallicity relation below the horizontal branch and applying it to multiple populations
Tim-Oliver Husser, Marilyn Latour, Jarle Brinchmann +7
Aims. We use the spectra of more than 30,000 red giant branch (RGB) stars in 25 globular clusters (GC), obtained within the MUSE survey of Galactic globular clusters, to calibrate…
MusE GAs FLOw and Wind (MEGAFLOW) IV: A two sightline tomography of a galactic wind
Johannes Zabl, Nicolas F. Bouché, Ilane Schroetter +8
Galactic outflows are thought to eject baryons back out to the circum-galactic medium (CGM). Studies based on metal absorption lines (MgII in particular) in the spectra of backgrou…
MUSEQuBES: Calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
Sowgat Muzahid, Joop Schaye, Raffaella Anna Marino +17
Lyman (Ly) emission lines are typically found to be redshifted with respect to the systemic redshifts of galaxies, likely due to resonant scattering of Ly photons. Here w…