papers

Publications (12)

astro-ph.GA2019

MusE GAs FLOw and Wind (MEGAFLOW) III: galactic wind properties using background quasars

Ilane Schroetter, Nicolas F. Bouché, Johannes Zabl +10

We present results from our on-going MusE GAs FLOw and Wind (MEGAFLOW) survey, which consists of 22 quasar lines-of-sight, each observed with the integral field unit (IFU) MUSE and…

astro-ph.GA2019

MusE GAs FLOw and Wind (MEGAFLOW) II. A study of gas accretion around star-forming galaxies with background quasars

Johannes Zabl, Nicolas F. Bouché, Ilane Schroetter +10

We use the MusE GAs FLOw and Wind (MEGAFLOW) survey to study the kinematics of extended disk-like structures of cold gas around star-forming galaxies. The combination o…

astro-ph.GA2015

The evolution of the stellar mass versus halo mass relationship

Peter Mitchell, Cedric Lacey, Carlton Baugh +1

We present an analysis of the predictions made by the Galform semi-analytic galaxy formation model for the evolution of the relationship between stellar mass and halo mass. We show…

astro-ph.IM2021

BlueMUSE: Project Overview and Science Cases

Johan Richard, Roland Bacon, Jérémy Blaizot +59

We present the concept of BlueMUSE, a blue-optimised, medium spectral resolution, panoramic integral field spectrograph based on the MUSE concept and proposed for the Very Large Te…

astro-ph.GA2021

Tracing the simulated high-redshift circum-galactic medium with Lyman alpha emission

Peter Mitchell, Jérémy Blaizot, Corentin Cadiou +3

With the Multi Unit Spectroscopic Explorer (MUSE), it is now possible to detect spatially extended Lyman alpha emission from individual faint (M_UV ~ -18) galaxies at redshifts, 3…

astro-ph.GA2017

The MUSE Hubble Ultra Deep Field Survey X. Ly Equivalent Widths at

Takuya Hashimoto, Thibault Garel, Bruno Guiderdoni +17

We present rest-frame Ly equivalent widths (EW) of 417 Ly emitters (LAEs) detected with Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT) at $2.9 <…

astro-ph.GA2017

The MUSE Hubble Ultra Deep Field Survey VIII : Extended Lyman-alpha haloes around high-redshift star-forming galaxies

Floriane Leclercq, Roland Bacon, Lutz Wisotzki +17

We report the detection of extended Lyman-alpha (Lya) haloes around 145 individual star-forming galaxies at redshifts 3<z<6 in the Hubble Ultra Deep Field observed with the Multi-U…

astro-ph.GA2018

The MUSE Hubble Ultra Deep Field Survey XI. Constraining the low-mass end of the stellar mass - star formation rate relation at

Leindert A. Boogaard, Jarle Brinchmann, Nicolas Bouché +16

Star-forming galaxies have been found to follow a relatively tight relation between stellar mass () and star formation rate (SFR), dubbed the `star formation sequence'. A tu…

astro-ph.GA2016

Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models

Quan Guo, Violeta Gonzalez-Perez, Qi Guo +12

We compare global predictions from the EAGLE hydrodynamical simulation, and two semi-analytic (SA) models of galaxy formation, L-GALAXIES and GALFORM. All three models include the…

quant-ph2002

Conditions for the confirmation of three-particle non-locality

Peter Mitchell, Sandu Popescu, David Roberts

The notion of genuine three-particle non-locality introduced by Svetlichny \cite{Svetlichny} is discussed. Svetlichny's inequality which can distinguish between genuine three-parti…

astro-ph.GA2020

The MUSE Hubble Ultra Deep Field Survey XIII. Spatially resolved spectral properties of Lyman alpha haloes around star-forming galaxies at z > 3

Floriane Leclercq, Roland Bacon, Anne Verhamme +18

We present spatially resolved maps of six individually-detected Lyman alpha haloes (LAHs) as well as a first statistical analysis of the Lyman alpha (Lya) spectral signature in the…

astro-ph.GA2017

Gas flows in the circumgalactic medium around simulated high-redshift galaxies

Peter Mitchell, Jeremy Blaizot, Julien Devriendt +4

We analyse the properties of circumgalactic gas around simulated galaxies in the redshift range z >= 3, utilising a new sample of cosmological zoom simulations. These simulations a…