activity
20172024
most citedThe MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

180 citations · 748 across the 18 of their papers we have counts for

collaborators

43 papers

astro-ph.GA20224 cited

ALMA as a Redshift Machine: Using [CII] to Efficiently Confirm Galaxies in the Epoch of Reionization

Sander Schouws, Rychard Bouwens, Renske Smit +11

The [CII] line has long been proposed as a promising line to spectroscopically confirm galaxies in the epoch of reionization. In this paper we present the results of new…

astro-ph.GA202127 cited

Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at

K. B. Schmidt, J. Kerutt, L. Wisotzki +17

[Abbreviated] Rest-frame UV emission lines probe physical parameters of the emitting star-forming galaxies and their environments. The strongest main UV line, Ly, has been instr…

astro-ph.GA202113 cited

The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman- emitters at

Y. Herrero Alonso, M. Krumpe, L. Wisotzki +12

We present an analysis of the spatial clustering of 695 Ly-emitting galaxies (LAE) in the MUSE-Wide survey. All objects have spectroscopically confirmed redshifts in the range $…

astro-ph.GA2021

The ALMA Spectroscopic Survey in the HUDF: A Search for [CII] Emitters at

Bade D. Uzgil, Pascal A. Oesch, Fabian Walter +18

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212-272 GHz) covers potential [CII] emission in galaxies at throughout a 2.9 arcm…

astro-ph.CO202177 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.GA20215 cited

Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy

M. Rybak, E. da Cunha, B. Groves +13

Extreme emission-line galaxies (EELGs) at redshift z=1-2 provide a unique view of metal-poor, starburst sources that are the likely drivers of the cosmic reionization at z.…