Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description

Michael L. Balogh; David G. Gilbank; Adam Muzzin; Gregory Rudnick; Chris Lidman; Andrea Biviano; Ricardo Demarco; Sean L. McGee; Julie B. Nantais; Allison Noble; Lyndsay Old; Gillian Wilson; Howard K. C. Yee; Callum Bellhouse; Pierluigi Cerulo; Jeffrey Chan; Irene Pintos-Castro; Rane Simpson; Remco F. J. van der Burg; Dennis Zaritsky; Felicia Ziparo; M. Victoria Alonso; Richard G. Bower; Gabriella De Lucia; Alexis Finoguenov; Diego Garcia Lambas; Hernan Muriel; Laura C. Parker; Alessandro Rettura; Carlos Valotto; Andrew Wetzel

doi:10.1093/mnras/stx1370

Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description

Michael L. Balogh, David G. Gilbank, Adam Muzzin, Gregory Rudnick, Chris Lidman, Andrea Biviano, Ricardo Demarco, Sean L. McGee, Julie B. Nantais, Allison Noble, Lyndsay Old, Gillian Wilson, Howard K. C. Yee, Callum Bellhouse, Pierluigi Cerulo, Jeffrey Chan, Irene Pintos-Castro, Rane Simpson, Remco F. J. van der Burg, Dennis ZaritskyFelicia Ziparo, M. Victoria Alonso, Richard G. Bower, Gabriella De Lucia, Alexis Finoguenov, Diego Garcia Lambas, Hernan Muriel, Laura C. Parker, Alessandro Rettura, Carlos Valotto, Andrew Wetzel

Physics and Astronomy

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Abstract

We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at $1z 10$ in halo mass. The scientific objectives include measuring the role of environment in the evolution of low-mass galaxies, and measuring the dynamics and stellar contents of their host haloes. The targets are selected from the SpARCS, SPT, COSMOS and SXDS surveys, to be the evolutionary counterparts of today's clusters and groups. The new red-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over $\lambda\sim 0.6$--$1.05\mu$m, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes $z^{\prime}[3.6]$\mu$m$

Original language	English
Journal	Royal Astronomical Society. Monthly Notices
Volume	470
Issue number	4
Early online date	3 Jun 2017
DOIs	https://doi.org/10.1093/mnras/stx1370
Publication status	E-pub ahead of print - 3 Jun 2017

Keywords

general – galaxies
evolution
galaxies
clusters

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10.1093/mnras/stx1370Licence: Creative Commons: Attribution (CC BY)

The_GOGREEN_survey_Monthly_Notices_2017Final published version, 5.26 MBLicence: Creative Commons: Attribution (CC BY)

Birmingham Astrophysics : Consolidated Grant 2013-2016
Vecchio, A., Ponman, T., Freise, A., Smith, G., Speake, C., Mandel, I., Cruise, M., Raychaudhury, S. & Stevens, I.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/13 → 30/09/16
Project: Research Councils

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Balogh, M. L., Gilbank, D. G., Muzzin, A., Rudnick, G., 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., Burg, R. F. J. V. D., ... Wetzel, A. (2017). Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description. Royal Astronomical Society. Monthly Notices, 470(4). Advance online publication. https://doi.org/10.1093/mnras/stx1370

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title = "Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description",

abstract = "We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at $1z 10$ in halo mass. The scientific objectives include measuring the role of environment in the evolution of low-mass galaxies, and measuring the dynamics and stellar contents of their host haloes. The targets are selected from the SpARCS, SPT, COSMOS and SXDS surveys, to be the evolutionary counterparts of today's clusters and groups. The new red-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over $\lambda\sim 0.6$--$1.05\mu$m, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes $z^{\prime}[3.6]$\mu$m$",

keywords = "general – galaxies, evolution, galaxies, clusters",

author = "Balogh, {Michael L.} and Gilbank, {David G.} and Adam Muzzin and Gregory Rudnick and Chris Lidman and Andrea Biviano and Ricardo Demarco and McGee, {Sean L.} and Nantais, {Julie B.} and Allison Noble and Lyndsay Old and Gillian Wilson and Yee, {Howard K. C.} and Callum Bellhouse and Pierluigi Cerulo and Jeffrey Chan and Irene Pintos-Castro and Rane Simpson and Burg, {Remco F. J. van der} and Dennis Zaritsky and Felicia Ziparo and Alonso, {M. Victoria} and Bower, {Richard G.} and Lucia, {Gabriella De} and Alexis Finoguenov and Lambas, {Diego Garcia} and Hernan Muriel and Parker, {Laura C.} and Alessandro Rettura and Carlos Valotto and Andrew Wetzel",

year = "2017",

month = jun,

day = "3",

doi = "10.1093/mnras/stx1370",

language = "English",

volume = "470",

journal = "Royal Astronomical Society. Monthly Notices",

issn = "0035-8711",

publisher = "SIPRI/Oxford University Press",

number = "4",

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Balogh, ML, Gilbank, DG, Muzzin, A, Rudnick, G, Lidman, C, Biviano, A, Demarco, R, McGee, SL, Nantais, JB, Noble, A, Old, L, Wilson, G, Yee, HKC, Bellhouse, C, Cerulo, P, Chan, J, Pintos-Castro, I, Simpson, R, Burg, RFJVD, Zaritsky, D, Ziparo, F, Alonso, MV, Bower, RG, Lucia, GD, Finoguenov, A, Lambas, DG, Muriel, H, Parker, LC, Rettura, A, Valotto, C & Wetzel, A 2017, 'Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description', Royal Astronomical Society. Monthly Notices, vol. 470, no. 4. https://doi.org/10.1093/mnras/stx1370

TY - JOUR

T1 - Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I

T2 - Survey Description

AU - Balogh, Michael L.

AU - Gilbank, David G.

AU - Muzzin, Adam

AU - Rudnick, Gregory

AU - Lidman, Chris

AU - Biviano, Andrea

AU - Demarco, Ricardo

AU - McGee, Sean L.

AU - Nantais, Julie B.

AU - Noble, Allison

AU - Old, Lyndsay

AU - Wilson, Gillian

AU - Yee, Howard K. C.

AU - Bellhouse, Callum

AU - Cerulo, Pierluigi

AU - Chan, Jeffrey

AU - Pintos-Castro, Irene

AU - Simpson, Rane

AU - Burg, Remco F. J. van der

AU - Zaritsky, Dennis

AU - Ziparo, Felicia

AU - Alonso, M. Victoria

AU - Bower, Richard G.

AU - Lucia, Gabriella De

AU - Finoguenov, Alexis

AU - Lambas, Diego Garcia

AU - Muriel, Hernan

AU - Parker, Laura C.

AU - Rettura, Alessandro

AU - Valotto, Carlos

AU - Wetzel, Andrew

PY - 2017/6/3

Y1 - 2017/6/3

N2 - We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at $1z 10$ in halo mass. The scientific objectives include measuring the role of environment in the evolution of low-mass galaxies, and measuring the dynamics and stellar contents of their host haloes. The targets are selected from the SpARCS, SPT, COSMOS and SXDS surveys, to be the evolutionary counterparts of today's clusters and groups. The new red-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over $\lambda\sim 0.6$--$1.05\mu$m, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes $z^{\prime}[3.6]$\mu$m$

AB - We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at $1z 10$ in halo mass. The scientific objectives include measuring the role of environment in the evolution of low-mass galaxies, and measuring the dynamics and stellar contents of their host haloes. The targets are selected from the SpARCS, SPT, COSMOS and SXDS surveys, to be the evolutionary counterparts of today's clusters and groups. The new red-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over $\lambda\sim 0.6$--$1.05\mu$m, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes $z^{\prime}[3.6]$\mu$m$

KW - general – galaxies

KW - evolution

KW - galaxies

KW - clusters

U2 - 10.1093/mnras/stx1370

DO - 10.1093/mnras/stx1370

M3 - Article

SN - 0035-8711

VL - 470

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

IS - 4

ER -

Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description

Abstract

Keywords

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Birmingham Astrophysics : Consolidated Grant 2013-2016

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