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19982025
most citedOverview of the DESI Legacy Imaging Surveys

1.9k citations · 14.1k across the 153 of their papers we have counts for

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Showing 2021 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2021★ 32 cited

Satellite quenching was not important for z1 clusters: most quenching occurred during infall

S. V. Werner, N. A. Hatch, A. Muzzin +4

We quantify the relative importance of environmental quenching versus pre-processing in clusters by analysing the infalling galaxy population in the outskirts of 15 galaxy…

astro-ph.GA2021★ 5 cited

H-based Star Formation Rates in and around z 0.5 EDisCS clusters

Jennifer R. Cooper, Gregory H. Rudnick, Gabriel G. Brammer +14

We investigate the role of environment on star-formation rates of galaxies at various cosmic densities in well-studied clusters. We present the star-forming main sequence for 163 g…

astro-ph.GA2021★ 36 cited

Virgo Filaments II: Catalog and First Results on the Effect of Filaments on galaxy properties

G. Castignani, B. Vulcani, R. A. Finn +12

Virgo is the nearest galaxy cluster; it is thus ideal for studies of galaxy evolution in dense environments in the local Universe. It is embedded in a complex filamentary network o…

astro-ph.GA2021★ 27 cited

HST/WFC3 grism observations of clusters: Evidence for rapid outside-in environmental quenching from spatially resolved H maps

Jasleen Matharu, Adam Muzzin, Gabriel B. Brammer +12

We present and publicly release (https://www.gclasshst.com) the first spatially resolved H maps of star-forming cluster galaxies at , made possible with the Wide Field C…

astro-ph.GA2021★ 36 cited

The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching

Karen McNab, Michael L. Balogh, Remco F. J. van der Burg +25

We measure the rate of environmentally-driven star formation quenching in galaxies at , using eleven massive () galaxy clusters…

astro-ph.GA2021★ 28 cited

The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching

Andrew M. M. Reeves, Michael L. Balogh, Remco F. J. van der Burg +18

We use photometric redshifts and statistical background subtraction to measure stellar mass functions in galaxy group-mass () haloes at $1<z<1.…