The miniJPAS survey: The role of group environment in quenching star formation

This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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Autores: González Delgado, Rosa M., Rodríguez-Martín, J. E., Díaz-García, L. A., García-Benito, Rubén, Martínez-Solaeche, Ginés, Pérez Jiménez, Enrique, Cid Fernandes, R., Hernán-Caballero, Antonio, Abramo, L. R., Alcaniz, Jailson, Benítez, Narciso, Bonoli, Silvia, Cenarro, A. J., Cristóbal-Hornillos, David, Diego, José María, Dupke, Renato A., Ederoclite, Alessandro, Fernández-Ontiveros, Juan Antonio, López-Sanjuan, Carlos, Marín-Franch, Antonio, Márquez, Isabel, Mendes de Oliveira, Claudia, Moles, Mariano, Pintos-Castro, Irene, Sodré, Laerte, Taylor, Keith, Varela, Jesús, Vázquez Ramió, H., Vílchez Medina, José Manuel
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2022
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/287713
Acceso en línea:http://hdl.handle.net/10261/287713
Access Level:acceso abierto
Palabra clave:Galaxies: evolution
Galaxies: stellar content
Galaxies: groups: general
Galaxies: photometry
Galaxies: fundamental parameters
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dc.title.none.fl_str_mv The miniJPAS survey: The role of group environment in quenching star formation
title The miniJPAS survey: The role of group environment in quenching star formation
spellingShingle The miniJPAS survey: The role of group environment in quenching star formation
González Delgado, Rosa M.
Galaxies: evolution
Galaxies: stellar content
Galaxies: groups: general
Galaxies: photometry
Galaxies: fundamental parameters
title_short The miniJPAS survey: The role of group environment in quenching star formation
title_full The miniJPAS survey: The role of group environment in quenching star formation
title_fullStr The miniJPAS survey: The role of group environment in quenching star formation
title_full_unstemmed The miniJPAS survey: The role of group environment in quenching star formation
title_sort The miniJPAS survey: The role of group environment in quenching star formation
dc.creator.none.fl_str_mv González Delgado, Rosa M.
Rodríguez-Martín, J. E.
Díaz-García, L. A.
García-Benito, Rubén
Martínez-Solaeche, Ginés
Pérez Jiménez, Enrique
Cid Fernandes, R.
Hernán-Caballero, Antonio
Abramo, L. R.
Alcaniz, Jailson
Benítez, Narciso
Bonoli, Silvia
Cenarro, A. J.
Cristóbal-Hornillos, David
Diego, José María
Dupke, Renato A.
Ederoclite, Alessandro
Fernández-Ontiveros, Juan Antonio
López-Sanjuan, Carlos
Marín-Franch, Antonio
Márquez, Isabel
Mendes de Oliveira, Claudia
Moles, Mariano
Pintos-Castro, Irene
Sodré, Laerte
Taylor, Keith
Varela, Jesús
Vázquez Ramió, H.
Vílchez Medina, José Manuel
author González Delgado, Rosa M.
author_facet González Delgado, Rosa M.
Rodríguez-Martín, J. E.
Díaz-García, L. A.
García-Benito, Rubén
Martínez-Solaeche, Ginés
Pérez Jiménez, Enrique
Cid Fernandes, R.
Hernán-Caballero, Antonio
Abramo, L. R.
Alcaniz, Jailson
Benítez, Narciso
Bonoli, Silvia
Cenarro, A. J.
Cristóbal-Hornillos, David
Diego, José María
Dupke, Renato A.
Ederoclite, Alessandro
Fernández-Ontiveros, Juan Antonio
López-Sanjuan, Carlos
Marín-Franch, Antonio
Márquez, Isabel
Mendes de Oliveira, Claudia
Moles, Mariano
Pintos-Castro, Irene
Sodré, Laerte
Taylor, Keith
Varela, Jesús
Vázquez Ramió, H.
Vílchez Medina, José Manuel
author_role author
author2 Rodríguez-Martín, J. E.
Díaz-García, L. A.
García-Benito, Rubén
Martínez-Solaeche, Ginés
Pérez Jiménez, Enrique
Cid Fernandes, R.
Hernán-Caballero, Antonio
Abramo, L. R.
Alcaniz, Jailson
Benítez, Narciso
Bonoli, Silvia
Cenarro, A. J.
Cristóbal-Hornillos, David
Diego, José María
Dupke, Renato A.
Ederoclite, Alessandro
Fernández-Ontiveros, Juan Antonio
López-Sanjuan, Carlos
Marín-Franch, Antonio
Márquez, Isabel
Mendes de Oliveira, Claudia
Moles, Mariano
Pintos-Castro, Irene
Sodré, Laerte
Taylor, Keith
Varela, Jesús
Vázquez Ramió, H.
Vílchez Medina, José Manuel
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
dc.contributor.none.fl_str_mv Ministerio de Ciencia e Innovación (España)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: evolution
Galaxies: stellar content
Galaxies: groups: general
Galaxies: photometry
Galaxies: fundamental parameters
topic Galaxies: evolution
Galaxies: stellar content
Galaxies: groups: general
Galaxies: photometry
Galaxies: fundamental parameters
description This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
publishDate 2022
dc.date.none.fl_str_mv 2022
2023
2023
dc.type.none.fl_str_mv info:eu-repo/semantics/article
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dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/287713
url http://hdl.handle.net/10261/287713
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spelling The miniJPAS survey: The role of group environment in quenching star formationGonzález Delgado, Rosa M.Rodríguez-Martín, J. E.Díaz-García, L. A.García-Benito, RubénMartínez-Solaeche, GinésPérez Jiménez, EnriqueCid Fernandes, R.Hernán-Caballero, AntonioAbramo, L. R.Alcaniz, JailsonBenítez, NarcisoBonoli, SilviaCenarro, A. J.Cristóbal-Hornillos, DavidDiego, José MaríaDupke, Renato A.Ederoclite, AlessandroFernández-Ontiveros, Juan AntonioLópez-Sanjuan, CarlosMarín-Franch, AntonioMárquez, IsabelMendes de Oliveira, ClaudiaMoles, MarianoPintos-Castro, IreneSodré, LaerteTaylor, KeithVarela, JesúsVázquez Ramió, H.Vílchez Medina, José ManuelGalaxies: evolutionGalaxies: stellar contentGalaxies: groups: generalGalaxies: photometryGalaxies: fundamental parametersThis is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.The miniJPAS survey has observed ∼1 deg2 of the AEGIS field with 60 bands (spectral resolution of R ∼ 60) in order to demonstrate the scientific potential of the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS), which will map ∼8000 deg2 of the northern sky over the coming years. In particular, this paper demonstrates the potential of J-PAS in detecting groups with mass of up to 1013 M⊙ and in characterising their galaxy populations up to z ∼ 1. The parametric code BaySeAGal is used to derive the stellar population properties by fitting the J-PAS spectral energy distribution (SED) of the galaxy members in 80 groups at z ≤ 0.8 previously detected by the AMICO code, and of a galaxy field sample retrieved from the whole miniJPAS down to r <  22.75 (AB). Blue, red, quiescent, and transition (blue quiescent or green valley) galaxy populations are identified through their rest-frame (extinction-corrected) (u − r)int colour, galaxy stellar mass (M⋆), and specific star formation rate (sSFR). We measure the abundance of these galaxies as a function of M⋆ and environment in order to investigate the role that groups play in quenching star formation. Our findings are as follows. (i) The fraction of red and quiescent galaxies in groups increases with M⋆ and is always higher in groups (28% on average) than in the field (5%). (ii) The quenched fraction excess (QFE) in groups shows a strong dependence on M⋆, and increases from a few percent for galaxies with M⋆ <  1010 M⊙ to higher than 60% for galaxies with M⋆ >  3 × 1011 M⊙. (iii) The abundance excess of transition galaxies in groups shows a modest dependence on M⋆, being 5%–10% for galaxies with M⋆ <  1011 M⊙. (iv) The fading timescale, defined as the time that galaxies in groups spend in the transition phase, is very short (< 1.5 Gyr), indicating that the star formation of galaxies in groups declines very rapidly. (v) The evolution of the galaxy quenching rate in groups shows a modest but significant evolution since z ∼ 0.8. This latter result is compatible with the expected evolution with constant QFE = 0.4, which has been previously measured for satellites in the nearby Universe, as traced by SDSS. Further, this evolution is consistent with a scenario where the low-mass star forming galaxies in clusters at z = 1–1.4 are environmentally quenched, as previously reported by other surveys. © R. M. González Delgado et al. 2022.R.G.D., L.A.D.G., R.G.B., G.M.S., J.R.M., and E.P. acknowledge financial support from the State Agency for Research of the Spanish MCIU through the ‘Center of Excellence Severo Ochoa’ award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709), and to PID2019-109067-GB100. I.M. acknowledges to PID2019-106027GB-C41. S.B. acknowledges to PGC2018-097585- B-C22, MINECO/FEDER, UE of the Spanish Ministerio de Economia, Industria y Competitividad. L.S.J. acknowledges the support from CNPq (304819/2017-4) and FAPESP (2019/10923-5). Based on observations made with the JST/T250 telescope and the Pathfinder camera for the miniJPAS project at the Observatorio Astrofísico de Javalambre (OAJ), in Teruel, owned, managed, and operated by the Centro de Estudios de Física del Cosmos de Aragón (CEFCA). We acknowledge the OAJ Data Processing and Archiving Unit (UPAD) for reducing and calibrating the OAJ data used in this work. Funding for OAJ, UPAD, and CEFCA has been provided by the Governments of Spain and Aragón through the Fondo de Inversiones de Teruel; the Aragón Government through the Research Groups E96, E103, and E16_17R; the Spanish Ministry of Science, Innovation and Universities (MCIU/AEI/FEDER, UE) with grant PGC2018-097585-B-C21; the Spanish Ministry of Economy and Competitiveness (MINECO/FEDER, UE) under AYA2015-66211-C2-1-P, AYA2015-66211-C2-2, AYA2012-30789, and ICTS-2009-14; and European FEDER funding (FCDD10-4E-867, FCDD13-4E-2685). J.A.F.O. acknowledges the financial support from the Spanish Ministry of Science and Innovation and the European Union – NextGenerationEU through the Recovery and Resilience Facility project ICTS-MRR-2021-03-CEFCA.Peer reviewedEDP SciencesMinisterio de Ciencia e Innovación (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202320232022info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/287713reponame:DIGITAL.CSIC. 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