Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane

Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC).

Detalles Bibliográficos
Autores: Díaz García, Luis Alberto, Cenarro, A. J., López Sanjuan, C., Peralta de Arriba, L., Ferreras, I., Cerviño, M., Márquez Pérez, Isabel, Masegosa, J., Del Olmo, A., Perea, J.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Institución:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/337
Acceso en línea:https://www.aanda.org/articles/aa/abs/2019/11/aa35257-19/aa35257-19.html
http://hdl.handle.net/20.500.12666/337
Access Level:acceso abierto
Palabra clave:Galaxies: stellar content
Galaxies: evolution
Galaxies: formation
Galaxies: photometry
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network_name_str España
repository_id_str
dc.title.none.fl_str_mv Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
title Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
spellingShingle Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
Díaz García, Luis Alberto
Galaxies: stellar content
Galaxies: evolution
Galaxies: formation
Galaxies: photometry
title_short Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
title_full Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
title_fullStr Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
title_full_unstemmed Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
title_sort Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size plane
dc.creator.none.fl_str_mv Díaz García, Luis Alberto
Cenarro, A. J.
López Sanjuan, C.
Peralta de Arriba, L.
Ferreras, I.
Cerviño, M.
Márquez Pérez, Isabel
Masegosa, J.
Del Olmo, A.
Perea, J.
author Díaz García, Luis Alberto
author_facet Díaz García, Luis Alberto
Cenarro, A. J.
López Sanjuan, C.
Peralta de Arriba, L.
Ferreras, I.
Cerviño, M.
Márquez Pérez, Isabel
Masegosa, J.
Del Olmo, A.
Perea, J.
author_role author
author2 Cenarro, A. J.
López Sanjuan, C.
Peralta de Arriba, L.
Ferreras, I.
Cerviño, M.
Márquez Pérez, Isabel
Masegosa, J.
Del Olmo, A.
Perea, J.
author2_role author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
Cerviño, M. [0000-0001-8009-231X]
De Arribas, L. P. [0000-0002-3084-084X]
López Sanjuan, C. [0000-0002-5743-3160]
Márquez Pérez, I. [0000-0003-2629-1945]
Gobierno de Aragón
Ministry of Science and Technology of Taiwan (MOST)
Academia Sinica
Ministerio de Ciencia e Innovación (MICINN)
Generalitat Valenciana
Junta de Andalucía
Generalitat de Catalunya
Ministerio de Economía y Competitividad (MINECO)
dc.subject.none.fl_str_mv Galaxies: stellar content
Galaxies: evolution
Galaxies: formation
Galaxies: photometry
topic Galaxies: stellar content
Galaxies: evolution
Galaxies: formation
Galaxies: photometry
description Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC).
publishDate 2019
dc.date.none.fl_str_mv 2019
2021
2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://www.aanda.org/articles/aa/abs/2019/11/aa35257-19/aa35257-19.html
http://hdl.handle.net/20.500.12666/337
url https://www.aanda.org/articles/aa/abs/2019/11/aa35257-19/aa35257-19.html
http://hdl.handle.net/20.500.12666/337
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv RESOLVIENDO LAS GALAXIAS EN ESPACIO Y TIEMPO: CLAVES PARA LA FORMACION Y EVOLUCION DE LAS GALAXIAS
info:eu-repo/grantAgreement/ES/MINECO/AYA2012-30789
GALAXIAS EN 3D A TRAVES DEL UNIVERSO: SINERGIA ENTRE ESPECTROSCOPIA DE CAMPO INTEGRAL Y CARTOGRAFIADOS MULTIBANDA PANORAMICOS
DESDE LAS BAJAS A LAS ALTAS TASAS DE ACRECION EN NUCLEOS ACTIVOS DE GALAXIAS. ALIMENTACION Y RETROALIMENTACION
EL PAPEL DE LAS FUSIONES EN LA FORMACION DE LAS GALAXIAS DE TIPO TEMPRANO Y SU CONEXION CON LA ACTIVIDAD NUCLEAR
CARTOGRAFIANDO EL CIELO: SONDEOS EN EL OPTICO E INFRARROJO DE LA VIA LACTEA
EVOLUCION DE GALAXIAS
WEAVE: EL ESPECTROGRAFO DE GRAN CAMPO DE NUEVA GENERACION PARA EL TELESCOPIO WILLIAM HERSCHEL
FORMACION Y EVOLUCION DE GALAXIAS EN 4D CON LOS CARTOGRAFIADOS MULTI-FILTRO J-PLUS Y J-PAS DESDE EL OAJ
EVOLUCION DE GALAXIAS
ACTIVIDAD NUCLEAR EN GALAXIAS
FORMACION ESTELAR VIOLENTA: LA RELACION ENTRE LAS ESTRELLAS Y EL GAS
DESARROLLO Y EXPLOTACION CIENTIFICA DEL OBSERVATORIO ASTROFISICO DE JAVALAMBRE: PRIMERA CIENCIA SOBRE EVOLUCION DE GALAXIAS Y COSMOLOGIA CON GRANDES CARTOGRAFIADOS
FORMACION DE GALAXIAS Y CUMULOS
ALHAMBRA: OBJETOS Y ESTRUCTURAS LEJANOS
EL PAPEL DE LOS ESTALLIDOS DE FORMACION ESTELAR EN LA FORMACION Y EVOLUCION DE GALAXIAS: ESTALLIDOS 5
info:eu-repo/grantAgreement/ES/MINECO/AYA2015-66211-C2-1-P
info:eu-repo/grantAgreement/MICINN//AYA2010-15081
info:eu-repo/grantAgreement/ES/MICINN/AYA2010-15169
info:eu-repo/grantAgreement/ES/MINECO/AYA2010-22111-C03-01
info:eu-repo/grantAgreement/MINECO//AYA2013-47742-C4-2-P
info:eu-repo/grantAgreement/ES/MINECO/AYA2010-22111-C03-02
info:eu-repo/grantAgreement/ES/MINECO/AYA2013-42227-P
info:eu-repo/grantAgreement/MINECO//AYA2011-29517-C03-01
info:eu-repo/grantAgreement/MINECO//AYA2013-43188-P
info:eu-repo/grantAgreement/MINECO//AYA2013-40611-P
info:eu-repo/grantAgreement/MINECO//AYA2014-57490-P
info:eu-repo/grantAgreement/MINECO//AYA2014-58861-C3-1-P
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/MINECO
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-76682-C3-3-P
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-77846-P
dc.rights.none.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
© ESO 2019
https://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
© ESO 2019
https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname:Instituto Nacional de Técnica Aeroespacial (INTA)
instname_str Instituto Nacional de Técnica Aeroespacial (INTA)
reponame_str DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
collection DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
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spelling Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1 IV. Properties of quiescent galaxies on the stellar mass–size planeDíaz García, Luis AlbertoCenarro, A. J.López Sanjuan, C.Peralta de Arriba, L.Ferreras, I.Cerviño, M.Márquez Pérez, IsabelMasegosa, J.Del Olmo, A.Perea, J.Galaxies: stellar contentGalaxies: evolutionGalaxies: formationGalaxies: photometryBased on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC).Aims. We perform a comprehensive study of the stellar population properties (formation epoch, age, metallicity, and extinction) of quiescent galaxies as a function of size and stellar mass to constrain the physical mechanism governing the stellar mass assembly and the likely evolutive scenarios that explain their growth in size. Methods. After selecting all the quiescent galaxies from the ALHAMBRA survey by the dust-corrected stellar mass–colour diagram, we built a shared sample of ∼850 quiescent galaxies with reliable measurements of sizes from the HST. This sample is complete in stellar mass and luminosity, I ≤ 23. The stellar population properties were retrieved using the fitting code for spectral energy distributions called MUlti-Filter FITting for stellar population diagnostics (MUFFIT) with various sets of composite stellar population models. Age, formation epoch, metallicity, and extinction were studied on the stellar mass–size plane as function of size through a Monte Carlo approach. This accounted for uncertainties and degeneracy effects amongst stellar population properties. Results. The stellar population properties of quiescent galaxies and their stellar mass and size since z ∼ 1 are correlated. At fixed stellar mass, the more compact the quiescent galaxy, the older and richer in metals it is (1 Gyr and 0.1 dex, respectively). In addition, more compact galaxies may present slight lower extinctions than their more extended counterparts at the same stellar mass (< 0.1 mag). By means of studying constant regions of stellar population properties across the stellar mass–size plane, we obtained empirical relations to constrain the physical mechanism that governs the stellar mass assembly of the form M⋆ ∝ rcα, where α amounts to 0.50–0.55 ± 0.09. There are indications that support the idea that the velocity dispersion is tightly correlated with the stellar content of galaxies. The mechanisms driving the evolution of stellar populations can therefore be partly linked to the dynamical properties of galaxies, along with their gravitational potential.This work has been supported by the Programa Nacional de Astronomia y Astrofisica of the Spanish Ministry of Economy and Competitiveness (MINECO, grants AYA2012-30789 and AYA2015-66211-C2-1-P), by the Government of Aragon (Research Group E103), by the Ministry of Science and Technology of Taiwan (grant MOST 106-2628-M-001-003MY3), and by the Academia Sinica (grant AS-IA-107-M01). The authors also acknowledge support from the Spanish Ministry for Economy and Competitiveness and FEDER funds through grants AYA2010-15081, AYA2010-15169, AYA2010-22111-C03-01, AYA2010-22111-C03-02, AYA2011-29517-C03-01, AYA2012-39620, AYA2013-40611-P, AYA2013-42227-P, AYA2013-43188-P, AYA2013-48623-C2-1, AYA2013-48623-C2-2, ESP2013-48274, AYA201457490-P, AYA2014-58861-C3-1, AYA2016-76682-C3-1-P, AYA2016-76682C3-3-P, AYA2016-77846-P Generalitat Valenciana projects Prometeo 2009/064 and PROMETEOII/2014/060, Junta de Andalucia grants TIC114, JA2828, P10FQM-6444, and Generalitat de Catalunya project SGR-1398. In this work we made use of the NYU Value Added Galaxy Catalogue DR7, which includes data from the Sloan Digital Sky Survey (SDSS) and the Two Micron All Sky Survey (2MASS). Funding for the SDSS has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the U.S. Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society. The SDSS Web site is http://www.sdss.org/.The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The Participating Institutions are The University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the MaxPlanck-Institute for Astrophysics (MPA), New Mexico State University, University of Pittsburgh, Princeton University, the United States Naval Observatory, and the University of Washington. This publication makes use of data products from the 2MASS, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. The authors thank the constructive and fruitful comments provided by the anonymous referee that surely helped to improve this paper. Throughout this research, we made use of the Matplotlib package (Hunter 2007), a 2D graphics package used for Python that is designed for interactive scripting and quality image generation. This paper is dedicated to Marian Leon Canalejo for being there when L.A.D.G. needed her most and for her patience and continuous encouragement while finishing his PhD.; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)Peer reviewEDP SciencesUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737Cerviño, M. [0000-0001-8009-231X]De Arribas, L. P. [0000-0002-3084-084X]López Sanjuan, C. [0000-0002-5743-3160]Márquez Pérez, I. [0000-0003-2629-1945]Gobierno de AragónMinistry of Science and Technology of Taiwan (MOST)Academia SinicaMinisterio de Ciencia e Innovación (MICINN)Generalitat ValencianaJunta de AndalucíaGeneralitat de CatalunyaMinisterio de Economía y Competitividad (MINECO)202120212019info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://www.aanda.org/articles/aa/abs/2019/11/aa35257-19/aa35257-19.htmlhttp://hdl.handle.net/20.500.12666/337reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)InglésRESOLVIENDO LAS GALAXIAS EN ESPACIO Y TIEMPO: CLAVES PARA LA FORMACION Y EVOLUCION DE LAS GALAXIASinfo:eu-repo/grantAgreement/ES/MINECO/AYA2012-30789GALAXIAS EN 3D A TRAVES DEL UNIVERSO: SINERGIA ENTRE ESPECTROSCOPIA DE CAMPO INTEGRAL Y CARTOGRAFIADOS MULTIBANDA PANORAMICOSDESDE LAS BAJAS A LAS ALTAS TASAS DE ACRECION EN NUCLEOS ACTIVOS DE GALAXIAS. ALIMENTACION Y RETROALIMENTACIONEL PAPEL DE LAS FUSIONES EN LA FORMACION DE LAS GALAXIAS DE TIPO TEMPRANO Y SU CONEXION CON LA ACTIVIDAD NUCLEARCARTOGRAFIANDO EL CIELO: SONDEOS EN EL OPTICO E INFRARROJO DE LA VIA LACTEAEVOLUCION DE GALAXIASWEAVE: EL ESPECTROGRAFO DE GRAN CAMPO DE NUEVA GENERACION PARA EL TELESCOPIO WILLIAM HERSCHELFORMACION Y EVOLUCION DE GALAXIAS EN 4D CON LOS CARTOGRAFIADOS MULTI-FILTRO J-PLUS Y J-PAS DESDE EL OAJEVOLUCION DE GALAXIASACTIVIDAD NUCLEAR EN GALAXIASFORMACION ESTELAR VIOLENTA: LA RELACION ENTRE LAS ESTRELLAS Y EL GASDESARROLLO Y EXPLOTACION CIENTIFICA DEL OBSERVATORIO ASTROFISICO DE JAVALAMBRE: PRIMERA CIENCIA SOBRE EVOLUCION DE GALAXIAS Y COSMOLOGIA CON GRANDES CARTOGRAFIADOSFORMACION DE GALAXIAS Y CUMULOSALHAMBRA: OBJETOS Y ESTRUCTURAS LEJANOSEL PAPEL DE LOS ESTALLIDOS DE FORMACION ESTELAR EN LA FORMACION Y EVOLUCION DE GALAXIAS: ESTALLIDOS 5info:eu-repo/grantAgreement/ES/MINECO/AYA2015-66211-C2-1-Pinfo:eu-repo/grantAgreement/MICINN//AYA2010-15081info:eu-repo/grantAgreement/ES/MICINN/AYA2010-15169info:eu-repo/grantAgreement/ES/MINECO/AYA2010-22111-C03-01info:eu-repo/grantAgreement/MINECO//AYA2013-47742-C4-2-Pinfo:eu-repo/grantAgreement/ES/MINECO/AYA2010-22111-C03-02info:eu-repo/grantAgreement/ES/MINECO/AYA2013-42227-Pinfo:eu-repo/grantAgreement/MINECO//AYA2011-29517-C03-01info:eu-repo/grantAgreement/MINECO//AYA2013-43188-Pinfo:eu-repo/grantAgreement/MINECO//AYA2013-40611-Pinfo:eu-repo/grantAgreement/MINECO//AYA2014-57490-Pinfo:eu-repo/grantAgreement/MINECO//AYA2014-58861-C3-1-Pinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/MINECOinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-76682-C3-3-Pinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-77846-PAttribution-NonCommercial-NoDerivatives 4.0 International© ESO 2019https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/3372026-06-23T12:46:37Z
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