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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

We compile a sample of spectroscopically and photometrically selected cluster galaxies from four high-redshift galaxy clusters (1.59 < z < 1.71) from the Spitzer Adaptation of the Red-Sequence Cluster Survey (SpARCS), and a comparison field sample selected from the UKIDSS Deep Survey. Using near-...


Delahaye, A.G.Webb, T.M.A.Nantais, J.Degroot, A.Wilson, G.Muzzin, A.Yee, H.K.C.Foltz, R.Noble, A.G.Demarco, R.Tudorica, A.Cooper, M.C.Lidman, C.Perlmutter, S.Hayden, B.Boone, K.Surace, J.[Galaxy Merger Candidates in High-redshift Cluster Environments]Galaxy Merger Candidates in High-redshift Cluster Environments

Context. Measuring and calibrating relations between cluster observables is critical for resource-limited studies. The mass-richness relation of clusters offers an observationally inexpensive way of estimating masses. Its calibration is essential for cluster and cosmological studies, especially f...


Tudorica, A.Hildebrandt, H.Tewes, M.Hoekstra, H.Morrison, C.B.Muzzin, A.Wilson, G.Yee, H.K.C.Lidman, C.Hicks, A.Nantais, J.Erben, T.Van Der Burg, R.F.J.Demarco, R.[Weak lensing magnification of SpARCS galaxy clusters]Weak lensing magnification of SpARCS galaxy clusters

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

We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z ∼ 1.6, constituting the largest sample of molecular gas measurements in z > 1.5 clusters to date. The observations span three galaxy clusters, derived from the Spitzer Adaptation of the Red-sequence Cluster Survey. We augmen...


Noble, A.G.McDonald, M.Muzzin, A.Nantais, J.Rudnick, G.Van Kampen, E.Webb, T.M.A.Wilson, G.Yee, H.K.C.Boone, K.Cooper, M.C.DeGroot, A.Delahaye, A.Demarco, R.Foltz, R.Hayden, B.Lidman, C.Manilla-Robles, A.Perlmutter, S.[ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments]ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments

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