Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
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 \(1
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| creator | Balogh, Michael L Gilbank, David G Muzzin, Adam Rudnick, Gregory Cooper, Michael C Lidman, Chris Biviano, Andrea Demarco, Ricardo McGee, Sean L Nantais, Julie B Noble, Allison Old, Lyndsay Wilson, Gillian Yee, Howard K C Bellhouse, Callum Cerulo, Pierluigi Chan, Jeffrey Pintos-Castro, Irene Simpson, Rane Remco F J van der Burg Zaritsky, Dennis Ziparo, Felicia Alonso, M Victoria Bower, Richard G Gabriella De Lucia Finoguenov, Alexis Diego Garcia Lambas Hernan Muriel Parker, Laura C Rettura, Alessandro Valotto, Carlos Wetzel, Andrew |
| description | 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 \(1 |
| doi_str_mv | 10.48550/arxiv.1705.01606 |
| format | Article |
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This is an imaging and deep spectroscopic survey of 21 galaxy systems at \(1<z<1.5\), selected to span a factor \(>10\) 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 \(z^{\prime}<24.25\) and [3.6]\(\mu\)m\(<22.5\), and is therefore statistically complete for stellar masses \(M_\ast\gtrsim10^{10.3}M_\odot\), for all galaxy types and over the entire redshift range. Deep, multiwavelength imaging has been acquired over larger fields for most systems, spanning \(u\) through \(K\), in addition to deep IRAC imaging at 3.6\(\mu\)m. The spectroscopy is \(\sim 50\) per cent complete as of semester 17A, and we anticipate a final sample of \(\sim 500\) new cluster members. Combined with existing spectroscopy on the brighter galaxies from GCLASS, SPT and other sources, GOGREEN will be a large legacy cluster and field galaxy sample at this redshift that spectroscopically covers a wide range in stellar mass, halo mass, and clustercentric radius.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1705.01606</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Galactic clusters ; Galactic evolution ; Galaxies ; Image acquisition ; Physics - Astrophysics of Galaxies ; Red shift ; Sky surveys (astronomy) ; Spectroscopy ; Spectrum analysis ; Stars & galaxies ; Stellar evolution ; Stellar mass ; Subtraction ; Telescopes</subject><ispartof>arXiv.org, 2017-06</ispartof><rights>2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1705.01606$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stx1370$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Balogh, Michael L</creatorcontrib><creatorcontrib>Gilbank, David G</creatorcontrib><creatorcontrib>Muzzin, Adam</creatorcontrib><creatorcontrib>Rudnick, Gregory</creatorcontrib><creatorcontrib>Cooper, Michael C</creatorcontrib><creatorcontrib>Lidman, Chris</creatorcontrib><creatorcontrib>Biviano, Andrea</creatorcontrib><creatorcontrib>Demarco, Ricardo</creatorcontrib><creatorcontrib>McGee, Sean L</creatorcontrib><creatorcontrib>Nantais, Julie B</creatorcontrib><creatorcontrib>Noble, Allison</creatorcontrib><creatorcontrib>Old, Lyndsay</creatorcontrib><creatorcontrib>Wilson, Gillian</creatorcontrib><creatorcontrib>Yee, Howard K C</creatorcontrib><creatorcontrib>Bellhouse, Callum</creatorcontrib><creatorcontrib>Cerulo, Pierluigi</creatorcontrib><creatorcontrib>Chan, Jeffrey</creatorcontrib><creatorcontrib>Pintos-Castro, Irene</creatorcontrib><creatorcontrib>Simpson, Rane</creatorcontrib><creatorcontrib>Remco F J van der Burg</creatorcontrib><creatorcontrib>Zaritsky, Dennis</creatorcontrib><creatorcontrib>Ziparo, Felicia</creatorcontrib><creatorcontrib>Alonso, M Victoria</creatorcontrib><creatorcontrib>Bower, Richard G</creatorcontrib><creatorcontrib>Gabriella De Lucia</creatorcontrib><creatorcontrib>Finoguenov, Alexis</creatorcontrib><creatorcontrib>Diego Garcia Lambas</creatorcontrib><creatorcontrib>Hernan Muriel</creatorcontrib><creatorcontrib>Parker, Laura C</creatorcontrib><creatorcontrib>Rettura, Alessandro</creatorcontrib><creatorcontrib>Valotto, Carlos</creatorcontrib><creatorcontrib>Wetzel, Andrew</creatorcontrib><title>Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description</title><title>arXiv.org</title><description>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 \(1<z<1.5\), selected to span a factor \(>10\) 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 \(z^{\prime}<24.25\) and [3.6]\(\mu\)m\(<22.5\), and is therefore statistically complete for stellar masses \(M_\ast\gtrsim10^{10.3}M_\odot\), for all galaxy types and over the entire redshift range. Deep, multiwavelength imaging has been acquired over larger fields for most systems, spanning \(u\) through \(K\), in addition to deep IRAC imaging at 3.6\(\mu\)m. The spectroscopy is \(\sim 50\) per cent complete as of semester 17A, and we anticipate a final sample of \(\sim 500\) new cluster members. Combined with existing spectroscopy on the brighter galaxies from GCLASS, SPT and other sources, GOGREEN will be a large legacy cluster and field galaxy sample at this redshift that spectroscopically covers a wide range in stellar mass, halo mass, and clustercentric radius.</description><subject>Galactic clusters</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Image acquisition</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Red shift</subject><subject>Sky surveys (astronomy)</subject><subject>Spectroscopy</subject><subject>Spectrum analysis</subject><subject>Stars & galaxies</subject><subject>Stellar evolution</subject><subject>Stellar mass</subject><subject>Subtraction</subject><subject>Telescopes</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotkE1PAjEURRsTEwnyA1zZxI0uBl8_X3FncBxJiCTIys2kM3ZiCXSwhQn8e0Fc3c3Jzb2HkBsGQ2mUgkcb974bMgQ1BKZBX5AeF4JlRnJ-RQYpLQGAa-RKiR75LNzaB09nVXKxs1vfhkTbhhZ2ZffeJeoDnfv6m-Y2rg40D52PbVi7sE30vpgV8zx_f6CTJ_qxi5070BeX6ug3p55rctnYVXKD_-yTxWu-GL9l01kxGT9PM6u4zJjSUjVWo6iE5gaxFgxdw2vDUcqKgdAjbLAyUI--kFcC8Ag1jNVgtXFa9MntufbveLmJfm3joTwJKP8EHIm7M7GJ7c_OpW25bHcxHDeVHFAZYCOU4hfYMVuG</recordid><startdate>20170627</startdate><enddate>20170627</enddate><creator>Balogh, Michael L</creator><creator>Gilbank, David G</creator><creator>Muzzin, Adam</creator><creator>Rudnick, Gregory</creator><creator>Cooper, Michael C</creator><creator>Lidman, Chris</creator><creator>Biviano, Andrea</creator><creator>Demarco, Ricardo</creator><creator>McGee, Sean L</creator><creator>Nantais, Julie B</creator><creator>Noble, Allison</creator><creator>Old, Lyndsay</creator><creator>Wilson, Gillian</creator><creator>Yee, Howard K C</creator><creator>Bellhouse, Callum</creator><creator>Cerulo, Pierluigi</creator><creator>Chan, Jeffrey</creator><creator>Pintos-Castro, Irene</creator><creator>Simpson, Rane</creator><creator>Remco F J van der Burg</creator><creator>Zaritsky, Dennis</creator><creator>Ziparo, Felicia</creator><creator>Alonso, M Victoria</creator><creator>Bower, Richard G</creator><creator>Gabriella De Lucia</creator><creator>Finoguenov, Alexis</creator><creator>Diego Garcia Lambas</creator><creator>Hernan Muriel</creator><creator>Parker, Laura C</creator><creator>Rettura, Alessandro</creator><creator>Valotto, Carlos</creator><creator>Wetzel, Andrew</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20170627</creationdate><title>Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description</title><author>Balogh, Michael L ; Gilbank, David G ; Muzzin, Adam ; Rudnick, Gregory ; Cooper, Michael C ; Lidman, Chris ; Biviano, Andrea ; Demarco, Ricardo ; McGee, Sean L ; Nantais, Julie B ; Noble, Allison ; Old, Lyndsay ; Wilson, Gillian ; Yee, Howard K C ; Bellhouse, Callum ; Cerulo, Pierluigi ; Chan, Jeffrey ; Pintos-Castro, Irene ; Simpson, Rane ; Remco F J van der Burg ; Zaritsky, Dennis ; Ziparo, Felicia ; Alonso, M Victoria ; Bower, Richard G ; Gabriella De Lucia ; Finoguenov, Alexis ; Diego Garcia Lambas ; Hernan Muriel ; Parker, Laura C ; Rettura, Alessandro ; Valotto, Carlos ; Wetzel, Andrew</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-15645fa673b362877c317ef2c82744b103697f7b80c9d72b307877f11c0a68e63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Galactic clusters</topic><topic>Galactic evolution</topic><topic>Galaxies</topic><topic>Image acquisition</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Red shift</topic><topic>Sky surveys (astronomy)</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><topic>Stars & galaxies</topic><topic>Stellar evolution</topic><topic>Stellar mass</topic><topic>Subtraction</topic><topic>Telescopes</topic><toplevel>online_resources</toplevel><creatorcontrib>Balogh, Michael L</creatorcontrib><creatorcontrib>Gilbank, David G</creatorcontrib><creatorcontrib>Muzzin, Adam</creatorcontrib><creatorcontrib>Rudnick, Gregory</creatorcontrib><creatorcontrib>Cooper, Michael C</creatorcontrib><creatorcontrib>Lidman, Chris</creatorcontrib><creatorcontrib>Biviano, Andrea</creatorcontrib><creatorcontrib>Demarco, Ricardo</creatorcontrib><creatorcontrib>McGee, Sean L</creatorcontrib><creatorcontrib>Nantais, Julie B</creatorcontrib><creatorcontrib>Noble, Allison</creatorcontrib><creatorcontrib>Old, Lyndsay</creatorcontrib><creatorcontrib>Wilson, Gillian</creatorcontrib><creatorcontrib>Yee, Howard K C</creatorcontrib><creatorcontrib>Bellhouse, Callum</creatorcontrib><creatorcontrib>Cerulo, Pierluigi</creatorcontrib><creatorcontrib>Chan, Jeffrey</creatorcontrib><creatorcontrib>Pintos-Castro, Irene</creatorcontrib><creatorcontrib>Simpson, Rane</creatorcontrib><creatorcontrib>Remco F J van der Burg</creatorcontrib><creatorcontrib>Zaritsky, Dennis</creatorcontrib><creatorcontrib>Ziparo, Felicia</creatorcontrib><creatorcontrib>Alonso, M Victoria</creatorcontrib><creatorcontrib>Bower, Richard G</creatorcontrib><creatorcontrib>Gabriella De Lucia</creatorcontrib><creatorcontrib>Finoguenov, Alexis</creatorcontrib><creatorcontrib>Diego Garcia Lambas</creatorcontrib><creatorcontrib>Hernan Muriel</creatorcontrib><creatorcontrib>Parker, Laura C</creatorcontrib><creatorcontrib>Rettura, Alessandro</creatorcontrib><creatorcontrib>Valotto, Carlos</creatorcontrib><creatorcontrib>Wetzel, Andrew</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest Central (New)</collection><collection>ProQuest One Academic (New)</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Middle East (New)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Applied & Life Sciences</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Balogh, Michael L</au><au>Gilbank, David G</au><au>Muzzin, Adam</au><au>Rudnick, Gregory</au><au>Cooper, Michael C</au><au>Lidman, Chris</au><au>Biviano, Andrea</au><au>Demarco, Ricardo</au><au>McGee, Sean L</au><au>Nantais, Julie B</au><au>Noble, Allison</au><au>Old, Lyndsay</au><au>Wilson, Gillian</au><au>Yee, Howard K C</au><au>Bellhouse, Callum</au><au>Cerulo, Pierluigi</au><au>Chan, Jeffrey</au><au>Pintos-Castro, Irene</au><au>Simpson, Rane</au><au>Remco F J van der Burg</au><au>Zaritsky, Dennis</au><au>Ziparo, Felicia</au><au>Alonso, M Victoria</au><au>Bower, Richard G</au><au>Gabriella De Lucia</au><au>Finoguenov, Alexis</au><au>Diego Garcia Lambas</au><au>Hernan Muriel</au><au>Parker, Laura C</au><au>Rettura, Alessandro</au><au>Valotto, Carlos</au><au>Wetzel, Andrew</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description</atitle><jtitle>arXiv.org</jtitle><date>2017-06-27</date><risdate>2017</risdate><eissn>2331-8422</eissn><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 \(1<z<1.5\), selected to span a factor \(>10\) 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 \(z^{\prime}<24.25\) and [3.6]\(\mu\)m\(<22.5\), and is therefore statistically complete for stellar masses \(M_\ast\gtrsim10^{10.3}M_\odot\), for all galaxy types and over the entire redshift range. Deep, multiwavelength imaging has been acquired over larger fields for most systems, spanning \(u\) through \(K\), in addition to deep IRAC imaging at 3.6\(\mu\)m. The spectroscopy is \(\sim 50\) per cent complete as of semester 17A, and we anticipate a final sample of \(\sim 500\) new cluster members. Combined with existing spectroscopy on the brighter galaxies from GCLASS, SPT and other sources, GOGREEN will be a large legacy cluster and field galaxy sample at this redshift that spectroscopically covers a wide range in stellar mass, halo mass, and clustercentric radius.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1705.01606</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Galactic clusters Galactic evolution Galaxies Image acquisition Physics - Astrophysics of Galaxies Red shift Sky surveys (astronomy) Spectroscopy Spectrum analysis Stars & galaxies Stellar evolution Stellar mass Subtraction Telescopes |
| title | Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description |
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