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arXiv · 2107.03425

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·Alexis Finoguenov·Egidijus Kukstas·Ian G. McCarthy·Kristi Webb·Adam Muzzin·Sean McGee·Gregory Rudnick·Andrea Biviano·Pierluigi Cerulo·Jeffrey C. C. Chan·M. C. Cooper·Ricardo Demarco·Pascale Jablonka·Gabriella De Lucia·Benedetta Vulcani·Gillian Wilson·Howard K. C. Yee·Dennis Zaritsky
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Abstract

We use photometric redshifts and statistical background subtraction to measure stellar mass functions in galaxy group-mass ($4.5-8\times10^{13}~\mathrm{M}_\odot$) haloes at $1 1$.

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Andrew M. M. Reeves, Michael L. Balogh, Remco F. J. van der Burg, Alexis Finoguenov, Egidijus Kukstas, Ian G. McCarthy, Kristi Webb, Adam Muzzin, Sean McGee, Gregory Rudnick, Andrea Biviano, Pierluigi Cerulo, Jeffrey C. C. Chan, M. C. Cooper, Ricardo Demarco, Pascale Jablonka, Gabriella De Lucia, Benedetta Vulcani, Gillian Wilson, Howard K. C. Yee, Dennis Zaritsky. 2021-07-07. The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching. https://doi.org/10.1093/mnras/stab1955

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