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...
| Autores: | , , , , , , , , , , , , , , , , , , , |
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| 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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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) |
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Universidad de Cantabria (UC) |
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UCrea Repositorio Abierto de la Universidad de Cantabria |
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UCrea Repositorio Abierto de la Universidad de Cantabria |
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15.811543 |