activity
19972022
most citedThe MUSE second-generation VLT instrument

879 citations · 5k across the 65 of their papers we have counts for

collaborators

65 papers

astro-ph.IM2022★ 879 cited

The MUSE second-generation VLT instrument

Bacon R., Accardo M., Adjali L. +65

The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation VLT panoramic integral-field spectrograph currently in manufacturing, assembly and integration phase. MUSE has a…

astro-ph.GA2022★ 44 cited

Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep

J. Kerutt, L. Wisotzki, A. Verhamme +15

The aim of this study is to better understand the connection between the Lyman rest-frame equivalent width (EW) and spectral properties as well as ultraviolet (UV) continuu…

astro-ph.CO2021★ 77 cited

The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift

Roland Bacon, David Mary, Thibault Garel +29

We report the discovery of diffuse extended Ly-alpha emission from redshift 3.1 to 4.5, tracing cosmic web filaments on scales of 2.5-4 comoving Mpc. These structures have been obs…

astro-ph.GA2020★ 84 cited

Search and analysis of giant radio galaxies with associated nuclei (SAGAN) -- I : New sample and multi-wavelength studies

Pratik Dabhade, Mousumi Mahato, Joydeep Bagchi +9

We present the first results of a project called SAGAN, which is dedicated solely to the studies of relatively rare megaparsec-scale radio galaxies in the Universe, called giant ra…

astro-ph.GA2020★ 1 cited

The MUSE Hubble Ultra Deep Field Survey XIV. The evolution of the Lya emitter fraction from z=3 to z=6

Haruka Kusakabe, Jeremy Blaizot, Thibault Garel +19

The Lya emitter (LAE) fraction, X_LAE, is a potentially powerful probe of the evolution of the intergalactic neutral hydrogen gas fraction. However, uncertainties in the measuremen…

astro-ph.GA2019★ 40 cited

Faint end of the luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE

G. de La Vieuville, D. Bina, R. Pello +21

We present the results obtained with VLT/MUSE on the faint-end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The precise aim of t…