The GOGREEN survey: transition galaxies and the evolution of environmental quenching

Research output: Working paper/PreprintPreprint


  • Karen McNab
  • Michael L. Balogh
  • Remco F. J. van der Burg
  • Anya Forestell
  • Kristi Webb
  • Benedetta Vulcani
  • Gregory Rudnick
  • Adam Muzzin
  • M. C. Cooper
  • Andrea Biviano
  • Pierluigi Cerulo
  • Jeffrey C. C. Chan
  • Gabriella De Lucia
  • Ricardo Demarco
  • Alexis Finoguenov
  • Ben Forrest
  • Caelan Golledge
  • Pascale Jablonka
  • Chris Lidman
  • Julie Nantais
  • Lyndsay Old
  • Irene Pintos-Castro
  • Bianca Poggianti
  • Andrew M. M. Reeves
  • Gillian Wilson
  • Howard K. C. Yee
  • Dennis Zaritsky

Colleges, School and Institutes


We measure the rate of environmentally-driven star formation quenching in galaxies at $z\sim 1$, using eleven massive ($M\approx 2\times10^{14}\,\mathrm{M}_\odot$) galaxy clusters spanning a redshift range $1.010.5$) we do not find any significant excess of transition galaxies in clusters, relative to a comparison field sample at the same redshift. It is likely that such galaxies were quenched prior to their accretion in the cluster, in group, filament or protocluster environments. For lower stellar mass galaxies ($9.5

Bibliographic note

Accepted for publication in MNRAS Sept 6, 2021


Original languageEnglish
Publication statusPublished - 7 Sep 2021


  • astro-ph.GA