Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description
- Autores
- 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; van der Burg, Remco; Zaritsky, Dennis; Ziparo, Felicia; Alonso, Maria Victoria; Bower, Richard G.; de Lucia, Gabriela Noemí; Finoguenov, Alexis; Garcia Lambas, Diego Rodolfo; Muriel, Hernan; Parker, Peter J.; Rettura, Alessandro; Valotto, Carlos Alberto; Wetzel, Andrew
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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 newred-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over λ ~ 0.6-1.05 μm, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes z' < 24.25 and [3.6] μm < 22.5, and is therefore statistically complete for stellar masses M* ≳ 1010.3M⊙, 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 μm. The spectroscopy is ~50 per cent complete as of semester 17A, and we anticipate a final sample of ~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.
Fil: Balogh, Michael L.. University of Waterloo; Canadá
Fil: Gilbank, David G.. South African Astronomical Observatory; Sudáfrica
Fil: Muzzin, Adam. University of York; Reino Unido
Fil: Rudnick, Gregory. University of Kansas; Estados Unidos
Fil: Cooper, Michael C.. University of California at Irvine; Estados Unidos
Fil: Lidman, Chris. Australian Astronomical Observatory; Australia
Fil: Biviano, Andrea. Osservatorio Astronomico Trieste; Italia
Fil: Demarco, Ricardo. Universidad de Concepción; Chile
Fil: McGee, Sean L.. University of Birmingham; Reino Unido
Fil: Nantais, Julie B.. Universidad Andrés Bello; Chile
Fil: Noble, Allison. Institute for Astrophysics and Space Research; Estados Unidos
Fil: Old, Lyndsay. University of Toronto; Canadá
Fil: Wilson, Gillian. University of California Riverside; Estados Unidos
Fil: Yee, Howard K. C.. University of Toronto; Canadá
Fil: Bellhouse, Callum. University of Birmingham; Reino Unido
Fil: Cerulo, Pierluigi. Universidad de Concepción; Chile
Fil: Chan, Jeffrey. University of California Riverside; Estados Unidos
Fil: Pintos-Castro, Irene. University of Toronto; Canadá
Fil: Simpson, Rane. University of Waterloo; Canadá
Fil: van der Burg, Remco. Université Paris Diderot - Paris 7; Francia
Fil: Zaritsky, Dennis. University of Arizona; Estados Unidos
Fil: Ziparo, Felicia. University of Birmingham; Reino Unido
Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Bower, Richard G.. University of Durham; Reino Unido
Fil: de Lucia, Gabriela Noemí. Osservatorio Astronomico di Trieste; Italia
Fil: Finoguenov, Alexis. Max-Planck-Institut; Alemania
Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Muriel, Hernan. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Parker, Peter J.. University of Hamilton; Canadá
Fil: Rettura, Alessandro. IPAC, Caltech; Estados Unidos
Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Wetzel, Andrew. University of California; Estados Unidos - Materia
-
CLUSTERS
EVOLUTION
GALAXIES
GENERAL-GALAXIES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/65188
Ver los metadatos del registro completo
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Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey descriptionBalogh, Michael L.Gilbank, David G.Muzzin, AdamRudnick, GregoryCooper, Michael C.Lidman, ChrisBiviano, AndreaDemarco, RicardoMcGee, Sean L.Nantais, Julie B.Noble, AllisonOld, LyndsayWilson, GillianYee, Howard K. C.Bellhouse, CallumCerulo, PierluigiChan, JeffreyPintos-Castro, IreneSimpson, Ranevan der Burg, RemcoZaritsky, DennisZiparo, FeliciaAlonso, Maria VictoriaBower, Richard G.de Lucia, Gabriela NoemíFinoguenov, AlexisGarcia Lambas, Diego RodolfoMuriel, HernanParker, Peter J.Rettura, AlessandroValotto, Carlos AlbertoWetzel, AndrewCLUSTERSEVOLUTIONGALAXIESGENERAL-GALAXIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We 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 newred-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over λ ~ 0.6-1.05 μm, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes z' < 24.25 and [3.6] μm < 22.5, and is therefore statistically complete for stellar masses M* ≳ 1010.3M⊙, 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 μm. The spectroscopy is ~50 per cent complete as of semester 17A, and we anticipate a final sample of ~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.Fil: Balogh, Michael L.. University of Waterloo; CanadáFil: Gilbank, David G.. South African Astronomical Observatory; SudáfricaFil: Muzzin, Adam. University of York; Reino UnidoFil: Rudnick, Gregory. University of Kansas; Estados UnidosFil: Cooper, Michael C.. University of California at Irvine; Estados UnidosFil: Lidman, Chris. Australian Astronomical Observatory; AustraliaFil: Biviano, Andrea. Osservatorio Astronomico Trieste; ItaliaFil: Demarco, Ricardo. Universidad de Concepción; ChileFil: McGee, Sean L.. University of Birmingham; Reino UnidoFil: Nantais, Julie B.. Universidad Andrés Bello; ChileFil: Noble, Allison. Institute for Astrophysics and Space Research; Estados UnidosFil: Old, Lyndsay. University of Toronto; CanadáFil: Wilson, Gillian. University of California Riverside; Estados UnidosFil: Yee, Howard K. C.. University of Toronto; CanadáFil: Bellhouse, Callum. University of Birmingham; Reino UnidoFil: Cerulo, Pierluigi. Universidad de Concepción; ChileFil: Chan, Jeffrey. University of California Riverside; Estados UnidosFil: Pintos-Castro, Irene. University of Toronto; CanadáFil: Simpson, Rane. University of Waterloo; CanadáFil: van der Burg, Remco. Université Paris Diderot - Paris 7; FranciaFil: Zaritsky, Dennis. University of Arizona; Estados UnidosFil: Ziparo, Felicia. University of Birmingham; Reino UnidoFil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Bower, Richard G.. University of Durham; Reino UnidoFil: de Lucia, Gabriela Noemí. Osservatorio Astronomico di Trieste; ItaliaFil: Finoguenov, Alexis. Max-Planck-Institut; AlemaniaFil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Muriel, Hernan. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Parker, Peter J.. University of Hamilton; CanadáFil: Rettura, Alessandro. IPAC, Caltech; Estados UnidosFil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Wetzel, Andrew. University of California; Estados UnidosWiley Blackwell Publishing, Inc2017-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/65188Balogh, Michael L.; Gilbank, David G.; Muzzin, Adam; Rudnick, Gregory; Cooper, Michael C.; et al.; Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 4; 10-2017; 4168-41850035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/reference/doi/10.1093/mnras/stx1370info:eu-repo/semantics/reference/url/https://academic.oup.com/mnrasinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1705.01606info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx1370info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/470/4/4168/3861119info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:00:50Zoai:ri.conicet.gov.ar:11336/65188instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-10 13:00:51.261CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| title |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| spellingShingle |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description Balogh, Michael L. CLUSTERS EVOLUTION GALAXIES GENERAL-GALAXIES |
| title_short |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| title_full |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| title_fullStr |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| title_full_unstemmed |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| title_sort |
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description |
| dc.creator.none.fl_str_mv |
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 van der Burg, Remco Zaritsky, Dennis Ziparo, Felicia Alonso, Maria Victoria Bower, Richard G. de Lucia, Gabriela Noemí Finoguenov, Alexis Garcia Lambas, Diego Rodolfo Muriel, Hernan Parker, Peter J. Rettura, Alessandro Valotto, Carlos Alberto Wetzel, Andrew |
| author |
Balogh, Michael L. |
| author_facet |
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 van der Burg, Remco Zaritsky, Dennis Ziparo, Felicia Alonso, Maria Victoria Bower, Richard G. de Lucia, Gabriela Noemí Finoguenov, Alexis Garcia Lambas, Diego Rodolfo Muriel, Hernan Parker, Peter J. Rettura, Alessandro Valotto, Carlos Alberto Wetzel, Andrew |
| author_role |
author |
| author2 |
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 van der Burg, Remco Zaritsky, Dennis Ziparo, Felicia Alonso, Maria Victoria Bower, Richard G. de Lucia, Gabriela Noemí Finoguenov, Alexis Garcia Lambas, Diego Rodolfo Muriel, Hernan Parker, Peter J. Rettura, Alessandro Valotto, Carlos Alberto Wetzel, Andrew |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
CLUSTERS EVOLUTION GALAXIES GENERAL-GALAXIES |
| topic |
CLUSTERS EVOLUTION GALAXIES GENERAL-GALAXIES |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
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 newred-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over λ ~ 0.6-1.05 μm, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes z' < 24.25 and [3.6] μm < 22.5, and is therefore statistically complete for stellar masses M* ≳ 1010.3M⊙, 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 μm. The spectroscopy is ~50 per cent complete as of semester 17A, and we anticipate a final sample of ~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. Fil: Balogh, Michael L.. University of Waterloo; Canadá Fil: Gilbank, David G.. South African Astronomical Observatory; Sudáfrica Fil: Muzzin, Adam. University of York; Reino Unido Fil: Rudnick, Gregory. University of Kansas; Estados Unidos Fil: Cooper, Michael C.. University of California at Irvine; Estados Unidos Fil: Lidman, Chris. Australian Astronomical Observatory; Australia Fil: Biviano, Andrea. Osservatorio Astronomico Trieste; Italia Fil: Demarco, Ricardo. Universidad de Concepción; Chile Fil: McGee, Sean L.. University of Birmingham; Reino Unido Fil: Nantais, Julie B.. Universidad Andrés Bello; Chile Fil: Noble, Allison. Institute for Astrophysics and Space Research; Estados Unidos Fil: Old, Lyndsay. University of Toronto; Canadá Fil: Wilson, Gillian. University of California Riverside; Estados Unidos Fil: Yee, Howard K. C.. University of Toronto; Canadá Fil: Bellhouse, Callum. University of Birmingham; Reino Unido Fil: Cerulo, Pierluigi. Universidad de Concepción; Chile Fil: Chan, Jeffrey. University of California Riverside; Estados Unidos Fil: Pintos-Castro, Irene. University of Toronto; Canadá Fil: Simpson, Rane. University of Waterloo; Canadá Fil: van der Burg, Remco. Université Paris Diderot - Paris 7; Francia Fil: Zaritsky, Dennis. University of Arizona; Estados Unidos Fil: Ziparo, Felicia. University of Birmingham; Reino Unido Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Bower, Richard G.. University of Durham; Reino Unido Fil: de Lucia, Gabriela Noemí. Osservatorio Astronomico di Trieste; Italia Fil: Finoguenov, Alexis. Max-Planck-Institut; Alemania Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Muriel, Hernan. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Parker, Peter J.. University of Hamilton; Canadá Fil: Rettura, Alessandro. IPAC, Caltech; Estados Unidos Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Wetzel, Andrew. University of California; Estados Unidos |
| 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 newred-sensitive Hamamatsu detectors on GMOS, coupled with the nod-and-shuffle sky subtraction, allow simultaneous wavelength coverage over λ ~ 0.6-1.05 μm, and this enables a homogeneous and statistically complete redshift survey of galaxies of all types. The spectroscopic sample targets galaxies with AB magnitudes z' < 24.25 and [3.6] μm < 22.5, and is therefore statistically complete for stellar masses M* ≳ 1010.3M⊙, 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 μm. The spectroscopy is ~50 per cent complete as of semester 17A, and we anticipate a final sample of ~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. |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017-10 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/65188 Balogh, Michael L.; Gilbank, David G.; Muzzin, Adam; Rudnick, Gregory; Cooper, Michael C.; et al.; Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 4; 10-2017; 4168-4185 0035-8711 1365-2966 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/65188 |
| identifier_str_mv |
Balogh, Michael L.; Gilbank, David G.; Muzzin, Adam; Rudnick, Gregory; Cooper, Michael C.; et al.; Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey description; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 4; 10-2017; 4168-4185 0035-8711 1365-2966 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/reference/doi/10.1093/mnras/stx1370 info:eu-repo/semantics/reference/url/https://academic.oup.com/mnras info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1705.01606 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx1370 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/470/4/4168/3861119 |
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openAccess |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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