activity
20172019
most citedThe MUSE-Wide survey: Detection of a clustering signal from Lyman-α-emitters at 3<z<6

17 citations · 17 across the 1 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2019

New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields

E. Ventou, T. Contini, N. Bouché +8

It is still a challenge to assess the merger fraction of galaxies at different cosmic epochs in order to probe the evolution of their mass assembly. Using the Illustris cosmologica…

astro-ph.GA2019

Spectral variations of Lyman-alpha emission within strongly lensed sources observed with MUSE

Adélaïde Claeyssens, Johan Richard, Jéméry Blaizot +13

We present an analysis of HI Lyman-alpha emission in deep VLT/MUSE observations of two highly magnified and extended galaxies at z=3.5 and 4.03, including a newly discovered, almos…

astro-ph.GA2019

Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z=1

V. Patrício, J. Richard, D. Carton +9

The existence of a spatially resolved Star-Forming Main Sequence (rSFMS) and a spatially resolved Mass-Metallicity Relation (rMZR) is now well established for local galaxies. Moreo…

astro-ph.GA2018

The MUSE-Wide Survey: Survey Description and First Data Release

T. Urrutia, L. Wisotzki, J. Kerutt +17

We present the MUSE-Wide survey, a blind, 3D spectroscopic survey in the CANDELS/GOODS-S and CANDELS/COSMOS regions. Each MUSE-Wide pointing has a depth of 1 hour and hence targets…

astro-ph.GA2018

The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last 10 Gyr

Alfred L. Tiley, A. M. Swinbank, C. M. Harrison +16

We analyse maps of the spatially-resolved nebular emission of 1500 star-forming galaxies at - from deep KMOS and MUSE observations to measure the average…

astro-ph.GA2018

Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies

L. Wisotzki, R. Bacon, J. Brinchmann +22

Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurement…