activity
20152021
most citedMulti-phase Circum-Galactic Medium probed with MUSE and ALMA

74 citations · 406 across the 10 of their papers we have counts for

collaborators

19 papers

astro-ph.GA202122 cited

Clumpiness of Observed and Simulated Cold Circumgalactic Gas

Ramona Augustin, Céline Péroux, Aleksandra Hamanowicz +3

Determining the clumpiness of matter around galaxies is pivotal to a full understanding of the spatially inhomogeneous, multi-phase gas in the circumgalactic medium (CGM). We combi…

astro-ph.GA202119 cited

MUSE-ALMA Halos VI: Coupling Atomic, Ionised & Molecular Gas Kinematics of Galaxies

Roland Szakacs, Céline Péroux, Martin Zwaan +7

We present results of MUSE-ALMA Halos, an ongoing study of the Circumgalactic Medium (CGM) of galaxies ( 1.4). Using multi-phase observations we probe the neutral, ionised…

astro-ph.GA2020

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…

astro-ph.GA201950 cited

MUSE-ALMA Halos V: Physical properties and environment of z < 1.4 HI quasar absorbers

A. Hamanowicz, C. Peroux, M. A. Zwaan +11

We present results of the MUSE-ALMA Halos, an ongoing study of the Circum-Galactic Medium (CGM) of low redshift galaxies (z < 1.4), currently comprising 14 strong HI absorbers in f…

astro-ph.GA201922 cited

Simulating MOS science on the ELT: Ly forest tomography

J. Japelj, C. Laigle, M. Puech +14

Mapping of the large-scale structure through cosmic time has numerous applications in the studies of cosmology and galaxy evolution. At , the structure can be traced by the…

astro-ph.GA201916 cited

Metal-enriched Galaxies in the First ~1 Billion Years: Evidence of a Smooth Metallicity Evolution at z ~ 5

Suraj Poudel, Varsha P. Kulkarni, Frances H. Cashman +4

We present seven new abundance measurements of the elements O, C and Si at z > 4.5, doubling the existing sample of weakly depleted elements in gas-rich galaxies, in order to const…