C. P'eroux

Cosmic web Lyα emission in a sample of overdense regions

We present a complete and homogeneous analysis of the łya emission properties of the cosmic web at 3 łesssim z łesssim 5 as a function of the overdensity of Lyα emitters (LAEs) in the MUSE Ultra Deep Field (MUDF) and the MUSE Extremely Deep Field (MXDF). We identified 41 overdensities, probing environments that are δ ≈...

MUSE-ALMA Haloes XVI: a census of the condensed baryons in z~0.5 HI absorption-selected galaxies

We use the MUSE-ALMA Haloes sample to build a census of the condensed baryons (stars and cold gas) to study the multiphase interstellar medium and circumgalactic medium (CGM). The sample includes 79 gas-rich galaxies at 0.2<z<1.2 located near strong HI Ly-alpha absorbers along quasar sightlines within projected separat...

MUSE-ALMA Haloes XV. Cold molecular, ionised, and stellar kinematics of HI-rich galaxies at z ∼ 0 . 5