GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment

Aims. In this paper, we revisit the data for the galaxy cluster ZwCl 0024.0+1652 provided by the GLACE survey and study the mass–metallicity function and its relationship with the environment. Methods. Here we describe an alternative way to reduce the data from OSIRIS tunable filters. This method gi...

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Autores: Cedrés, Bernabé, De Daniloff, Simon B., Bongiovanni, Ángel, Sánchez-Portal, Miguel, Cerviño, Miguel, Pérez-Martínez, Ricardo, Pérez-García, Ana María, Cepa, Jordi, Lara-López, Maritza A., González-Otero, Mauro, Castillo-Fraile, Manuel, González Serrano, José Ignacio|||0000-0003-0795-3026, Negrete, Castalia Alenka, Padilla-Torres, Camen P., Pintos-Castro, Irene, Povic, Mirjana, Alfaro, Emilio, Beyoro-Amado, Zeleke, Cruz-González, Irene, Diego, José A. de
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universidad de Cantabria (UC)
Repositorio:UCrea Repositorio Abierto de la Universidad de Cantabria
Idioma:inglés
OAI Identifier:oai:repositorio.unican.es:10902/35329
Acceso en línea:https://hdl.handle.net/10902/35329
Access Level:acceso abierto
Palabra clave:ISM: abundances
Galaxies: clusters: individual: ZwCl 0024.0+1652
Galaxies: star formation
Cosmology: observations
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spelling GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environmentCedrés, BernabéDe Daniloff, Simon B.Bongiovanni, ÁngelSánchez-Portal, MiguelCerviño, MiguelPérez-Martínez, RicardoPérez-García, Ana MaríaCepa, JordiLara-López, Maritza A.González-Otero, MauroCastillo-Fraile, ManuelGonzález Serrano, José Ignacio|||0000-0003-0795-3026Negrete, Castalia AlenkaPadilla-Torres, Camen P.Pintos-Castro, IrenePovic, MirjanaAlfaro, EmilioBeyoro-Amado, ZelekeCruz-González, IreneDiego, José A. deISM: abundancesGalaxies: clusters: individual: ZwCl 0024.0+1652Galaxies: star formationCosmology: observationsAims. In this paper, we revisit the data for the galaxy cluster ZwCl 0024.0+1652 provided by the GLACE survey and study the mass–metallicity function and its relationship with the environment. Methods. Here we describe an alternative way to reduce the data from OSIRIS tunable filters. This method gives us better uncertainties in the fluxes of the emission lines and the derived quantities. We present an updated catalogue of cluster galaxies with emission in Hα and [N II] λλ6548,6583. We also discuss the biases of these new fluxes and describe the way in which we calculated the mass–metallicity relationship and its uncertainties. Results. We generated a new catalogue of 84 emission-line galaxies with reliable fluxes in [N II] and Hα lines from a list of 174 galaxies. We find a relationship between the clustercentric radius and the density of galaxies. We derived the mass–metallicity relationship for ZwCl 0024.0+1652 and compared it with clusters and field galaxies from the literature. We find a difference in the mass–metallicity relationship when compared to more massive clusters, with the latter showing on average higher values of abundance. This could be an effect of the quenching of the star formation, which seems to be more prevalent in low-mass galaxies in more massive clusters. We find little to no difference between ZwCl 0024.0+1652 galaxies and field galaxies located at the same redshift.B.C., M.S.P., and A.B. acknowledge the support of the Spanish Ministry of Science, Innovation and Universities through the project PID-2021-122544NB-C43. J.C. and M.G.-O. acknowledges the support of the Spanish Ministry of Science, Innovation and Universities through the project PID-2021-122544NB-C41. M.A.L.L. acknowledges support from the Spanish grant PID-2021-123417OB-I00, and the Ramón y Cajal program funded by the Spanish Government (RYC2020-029354-I). M.C. acknowledges the support of PID2019-107408GB-C41 and PID2022-136598NB-C33 grants funded by MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”.EDP SciencesUniversidad de Cantabria20242024-06-01journal articlehttp://purl.org/coar/resource_type/c_6501NAhttp://purl.org/coar/version/c_be7fb7dd8ff6fe43info:eu-repo/semantics/articlehttps://hdl.handle.net/10902/35329Astronomy & Astrophysics, 2024, 686, A60reponame:UCrea Repositorio Abierto de la Universidad de Cantabriainstname:Universidad de Cantabria (UC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.unican.es:10902/353292026-06-02T12:39:31Z
dc.title.none.fl_str_mv GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
title GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
spellingShingle GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
Cedrés, Bernabé
ISM: abundances
Galaxies: clusters: individual: ZwCl 0024.0+1652
Galaxies: star formation
Cosmology: observations
title_short GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
title_full GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
title_fullStr GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
title_full_unstemmed GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
title_sort GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652: II. The mass-metallicity relationship and the effect of the environment
dc.creator.none.fl_str_mv Cedrés, Bernabé
De Daniloff, Simon B.
Bongiovanni, Ángel
Sánchez-Portal, Miguel
Cerviño, Miguel
Pérez-Martínez, Ricardo
Pérez-García, Ana María
Cepa, Jordi
Lara-López, Maritza A.
González-Otero, Mauro
Castillo-Fraile, Manuel
González Serrano, José Ignacio|||0000-0003-0795-3026
Negrete, Castalia Alenka
Padilla-Torres, Camen P.
Pintos-Castro, Irene
Povic, Mirjana
Alfaro, Emilio
Beyoro-Amado, Zeleke
Cruz-González, Irene
Diego, José A. de
author Cedrés, Bernabé
author_facet Cedrés, Bernabé
De Daniloff, Simon B.
Bongiovanni, Ángel
Sánchez-Portal, Miguel
Cerviño, Miguel
Pérez-Martínez, Ricardo
Pérez-García, Ana María
Cepa, Jordi
Lara-López, Maritza A.
González-Otero, Mauro
Castillo-Fraile, Manuel
González Serrano, José Ignacio|||0000-0003-0795-3026
Negrete, Castalia Alenka
Padilla-Torres, Camen P.
Pintos-Castro, Irene
Povic, Mirjana
Alfaro, Emilio
Beyoro-Amado, Zeleke
Cruz-González, Irene
Diego, José A. de
author_role author
author2 De Daniloff, Simon B.
Bongiovanni, Ángel
Sánchez-Portal, Miguel
Cerviño, Miguel
Pérez-Martínez, Ricardo
Pérez-García, Ana María
Cepa, Jordi
Lara-López, Maritza A.
González-Otero, Mauro
Castillo-Fraile, Manuel
González Serrano, José Ignacio|||0000-0003-0795-3026
Negrete, Castalia Alenka
Padilla-Torres, Camen P.
Pintos-Castro, Irene
Povic, Mirjana
Alfaro, Emilio
Beyoro-Amado, Zeleke
Cruz-González, Irene
Diego, José A. de
author2_role 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 Universidad de Cantabria
dc.subject.none.fl_str_mv ISM: abundances
Galaxies: clusters: individual: ZwCl 0024.0+1652
Galaxies: star formation
Cosmology: observations
topic ISM: abundances
Galaxies: clusters: individual: ZwCl 0024.0+1652
Galaxies: star formation
Cosmology: observations
description Aims. In this paper, we revisit the data for the galaxy cluster ZwCl 0024.0+1652 provided by the GLACE survey and study the mass–metallicity function and its relationship with the environment. Methods. Here we describe an alternative way to reduce the data from OSIRIS tunable filters. This method gives us better uncertainties in the fluxes of the emission lines and the derived quantities. We present an updated catalogue of cluster galaxies with emission in Hα and [N II] λλ6548,6583. We also discuss the biases of these new fluxes and describe the way in which we calculated the mass–metallicity relationship and its uncertainties. Results. We generated a new catalogue of 84 emission-line galaxies with reliable fluxes in [N II] and Hα lines from a list of 174 galaxies. We find a relationship between the clustercentric radius and the density of galaxies. We derived the mass–metallicity relationship for ZwCl 0024.0+1652 and compared it with clusters and field galaxies from the literature. We find a difference in the mass–metallicity relationship when compared to more massive clusters, with the latter showing on average higher values of abundance. This could be an effect of the quenching of the star formation, which seems to be more prevalent in low-mass galaxies in more massive clusters. We find little to no difference between ZwCl 0024.0+1652 galaxies and field galaxies located at the same redshift.
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-06-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
NA
http://purl.org/coar/version/c_be7fb7dd8ff6fe43
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/10902/35329
url https://hdl.handle.net/10902/35329
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv Astronomy & Astrophysics, 2024, 686, A60
reponame:UCrea Repositorio Abierto de la Universidad de Cantabria
instname:Universidad de Cantabria (UC)
instname_str Universidad de Cantabria (UC)
reponame_str UCrea Repositorio Abierto de la Universidad de Cantabria
collection UCrea Repositorio Abierto de la Universidad de Cantabria
repository.name.fl_str_mv
repository.mail.fl_str_mv
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