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

Karen McNab; Michael L. Balogh; Remco F. J. van der Burg; Anya Forestell; Kristi Webb; Benedetta Vulcani; Gregory Rudnick; Adam Muzzin; M. C. Cooper; Sean McGee; 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

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

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

Physics and Astronomy

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Abstract

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

Original language	English
Publication status	Published - 7 Sept 2021

Bibliographical note

Accepted for publication in MNRAS Sept 6, 2021

Keywords

astro-ph.GA

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2109.03105v1Other version, 1.65 MBLicence: None: All rights reserved

https://arxiv.org/abs/2109.03105Licence: None: All rights reserved

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McNab, K., Balogh, M. L., Burg, R. F. J. V. D., Forestell, A., Webb, K., Vulcani, B., Rudnick, G., Muzzin, A., Cooper, M. C., McGee, S., Biviano, A., Cerulo, P., Chan, J. C. C., Lucia, G. D., Demarco, R., Finoguenov, A., Forrest, B., Golledge, C., Jablonka, P., ... Zaritsky, D. (2021). The GOGREEN survey: transition galaxies and the evolution of environmental quenching. https://arxiv.org/abs/2109.03105

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title = "The GOGREEN survey: transition galaxies and the evolution of environmental quenching",

abstract = " 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",

keywords = "astro-ph.GA",

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

note = "Accepted for publication in MNRAS Sept 6, 2021",

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day = "7",

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type = "WorkingPaper",

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McNab, K, Balogh, ML, Burg, RFJVD, Forestell, A, Webb, K, Vulcani, B, Rudnick, G, Muzzin, A, Cooper, MC, McGee, S, Biviano, A, Cerulo, P, Chan, JCC, Lucia, GD, Demarco, R, Finoguenov, A, Forrest, B, Golledge, C, Jablonka, P, Lidman, C, Nantais, J, Old, L, Pintos-Castro, I, Poggianti, B, Reeves, AMM, Wilson, G, Yee, HKC & Zaritsky, D 2021 'The GOGREEN survey: transition galaxies and the evolution of environmental quenching'. <https://arxiv.org/abs/2109.03105>

TY - UNPB

T1 - The GOGREEN survey: transition galaxies and the evolution of environmental quenching

AU - McNab, Karen

AU - Balogh, Michael L.

AU - Burg, Remco F. J. van der

AU - Forestell, Anya

AU - Webb, Kristi

AU - Vulcani, Benedetta

AU - Rudnick, Gregory

AU - Muzzin, Adam

AU - Cooper, M. C.

AU - McGee, Sean

AU - Biviano, Andrea

AU - Cerulo, Pierluigi

AU - Chan, Jeffrey C. C.

AU - Lucia, Gabriella De

AU - Demarco, Ricardo

AU - Finoguenov, Alexis

AU - Forrest, Ben

AU - Golledge, Caelan

AU - Jablonka, Pascale

AU - Lidman, Chris

AU - Nantais, Julie

AU - Old, Lyndsay

AU - Pintos-Castro, Irene

AU - Poggianti, Bianca

AU - Reeves, Andrew M. M.

AU - Wilson, Gillian

AU - Yee, Howard K. C.

AU - Zaritsky, Dennis

N1 - Accepted for publication in MNRAS Sept 6, 2021

PY - 2021/9/7

Y1 - 2021/9/7

N2 - 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

AB - 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

KW - astro-ph.GA

UR - https://doi.org/10.1093/mnras/stab2558

M3 - Preprint

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

ER -

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

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