Stellar mass function of cluster galaxies at z ~ 1.5: evidence for reduced quenching efficiency at high redshift
A&A, 592 (2016) A161
Published online: 2016-08-24
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The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching
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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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Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description
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Evidence for strong evolution in galaxy environmental quenching efficiency betweenz= 1.6 andz= 0.9
Julie B. Nantais, Adam Muzzin, Remco F. J. van der Burg, et al.Monthly Notices of the Royal Astronomical Society: Letters 465 (1) L104 (2017)
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Galaxy Merger Candidates in High-redshift Cluster Environments
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The Ages of Passive Galaxies in a z = 1.62 Protocluster
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Star-rich early galaxy clusters
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