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We analyse the evolution of environmental quenching efficiency, the fraction of quenched cluster galaxies which would be star forming if they were in the field, as a function of redshift in 14 spectroscopically confirmed galaxy clusters with 0.87 < z < 1.63 from the Spitzer Adaptation of the Red-...


Nantais, J.B.Muzzin, A.van der Burg, R.F.J.Wilson, G.Lidman, C.Foltz, R.DeGroot, A.Noble, A.Cooper, M.C.Demarco, R.[Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9]Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9

Balogh, M.L.Gilbank, D.G.Muzzin, A.Rudnick, G.Cooper, M.C.Lidman, C.Biviano, A.Demarco, R.McGee, S.L.Nantais, J.B.Noble, A.Old, L.Wilson, G.Yee, H.K.C.Bellhouse, C.Cerulo, P.Chan, J.Pintos-Castro, I.Simpson, R.van der Burg, R.F.J.Zaritsky, D.Ziparo, F.Alonso, M.V.Bower, R.G.Lucia, G.D.Finoguenov, A.Lambas, D.G.Muriel, H.Parker, L.C.Rettura, A.Valotto, C.Wetzel, A.[Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description]Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description

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