activity
19972022
most citedUV Star Formation Rates in the Local Universe

1.7k citations · 5.3k across the 41 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

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.GA2019

GALEX colours of quasars and intergalactic medium opacity at low redshift

J. -M. Deharveng, B. Milliard, C. Peroux +1

The distribution of neutral hydrogen in the intergalactic medium (IGM) is currently explored at low-z by means of UV spectroscopy of quasars. We propose an alternative approach bas…

astro-ph.GA2019

Emission from the circumgalactic medium: from cosmological zoom-in simulations to multiwavelength observables

R. Augustin, S. Quiret, B. Milliard +14

We simulate the flux emitted from galaxy halos in order to quantify the brightness of the circumgalactic medium (CGM). We use dedicated zoom-in cosmological simulations with the hy…

astro-ph.GA201974 cited

Multi-phase Circum-Galactic Medium probed with MUSE and ALMA

Celine Peroux, Martin Zwaan, Anne Klitsch +9

Galaxy halos appear to be missing a large fraction of their baryons, most probably hiding in the circumgalactic medium (CGM), a diffuse component within the dark matter halo that e…

astro-ph.GA2018

A Lyman limit system associated with galactic winds

Hadi Rahmani, Celine Peroux, Ilane Schroetter +9

Projected quasar galaxy pairs provide powerful means to study the circumgalactic medium (CGM) that maintains the relics of galactic feedback and the accreted gas from the intergala…

astro-ph.GA2018

Characterising the Circum-Galactic Medium of Damped Lyman- Absorbing Galaxies

Ramona Augustin, Celine Peroux, Palle Moller +8

Gas flows in and out of galaxies through their circumgalactic medium (CGM) are poorly constrained and direct observations of this faint, diffuse medium remain challenging. We use a…