The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies

Autores
Rodriguez, Facundo; Montero Dorta, Antonio D.; Angulo, Raul E.; Artale, Maria Celeste; Merchan, Manuel Enrique
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez & Merchán in order to determine the stellar and halo mass-size relations of central and satellite galaxies separately. We show that, while central and satellite galaxies display similar stellar mass-size relations, their halo mass-size relations differ significantly. As expected, more massive haloes tend to host larger central galaxies. However, the size of satellite galaxies depends only slightly on halo virial mass. We show that these results are compatible with a remarkably simple model in which the size of central and satellite galaxies scales as the cubic root of their host halo mass, with the normalization for satellites being ∼30 per cent smaller than that for central galaxies, which can be attributed to tidal stripping. We further check that our measurements are in excellent agreement with predictions from the IllustrisTNG hydrodynamical simulation. In the second part of this paper, we analyse how the clustering properties of central and satellite galaxies depend on their size. We demonstrate that, independently of the stellar mass threshold adopted, smaller galaxies are more tightly clustered than larger galaxies when either the entire sample or only satellites are considered. The opposite trend is observed on large scales when the size split is performed for the central galaxies alone. Our results place significant constraints for halo-galaxy connection models that link galaxy size with the properties of their hosting haloes.
Fil: Rodriguez, Facundo. 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: Montero Dorta, Antonio D.. Universidade de Sao Paulo; Brasil. Universidad Técnica Federico Santa María; Chile
Fil: Angulo, Raul E.. Ikerbasque, Basque Foundation For Science; España. Donostia International Physics Center; España
Fil: Artale, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Innsbruck; Austria
Fil: Merchan, Manuel Enrique. 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
Materia
LARGE-SCALE STRUCTURE OF UNIVERSE
GALAXIES: STATISTICS
GALAXIES: GROUPS
GALAXIES: HALOES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/170944
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/170944
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxiesRodriguez, FacundoMontero Dorta, Antonio D.Angulo, Raul E.Artale, Maria CelesteMerchan, Manuel EnriqueLARGE-SCALE STRUCTURE OF UNIVERSEGALAXIES: STATISTICSGALAXIES: GROUPSGALAXIES: HALOEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez & Merchán in order to determine the stellar and halo mass-size relations of central and satellite galaxies separately. We show that, while central and satellite galaxies display similar stellar mass-size relations, their halo mass-size relations differ significantly. As expected, more massive haloes tend to host larger central galaxies. However, the size of satellite galaxies depends only slightly on halo virial mass. We show that these results are compatible with a remarkably simple model in which the size of central and satellite galaxies scales as the cubic root of their host halo mass, with the normalization for satellites being ∼30 per cent smaller than that for central galaxies, which can be attributed to tidal stripping. We further check that our measurements are in excellent agreement with predictions from the IllustrisTNG hydrodynamical simulation. In the second part of this paper, we analyse how the clustering properties of central and satellite galaxies depend on their size. We demonstrate that, independently of the stellar mass threshold adopted, smaller galaxies are more tightly clustered than larger galaxies when either the entire sample or only satellites are considered. The opposite trend is observed on large scales when the size split is performed for the central galaxies alone. Our results place significant constraints for halo-galaxy connection models that link galaxy size with the properties of their hosting haloes.Fil: Rodriguez, Facundo. 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: Montero Dorta, Antonio D.. Universidade de Sao Paulo; Brasil. Universidad Técnica Federico Santa María; ChileFil: Angulo, Raul E.. Ikerbasque, Basque Foundation For Science; España. Donostia International Physics Center; EspañaFil: Artale, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Innsbruck; AustriaFil: Merchan, Manuel Enrique. 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; ArgentinaOxford University Press2021-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/170944Rodriguez, Facundo; Montero Dorta, Antonio D.; Angulo, Raul E.; Artale, Maria Celeste; Merchan, Manuel Enrique; The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 505; 3; 8-2021; 3192-32050035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab1571/6289926info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab1571info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:10:16Zoai:ri.conicet.gov.ar:11336/170944instacron: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:34982025-09-29 10:10:16.401CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
title The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
spellingShingle The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
Rodriguez, Facundo
LARGE-SCALE STRUCTURE OF UNIVERSE
GALAXIES: STATISTICS
GALAXIES: GROUPS
GALAXIES: HALOES
title_short The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
title_full The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
title_fullStr The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
title_full_unstemmed The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
title_sort The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
dc.creator.none.fl_str_mv Rodriguez, Facundo
Montero Dorta, Antonio D.
Angulo, Raul E.
Artale, Maria Celeste
Merchan, Manuel Enrique
author Rodriguez, Facundo
author_facet Rodriguez, Facundo
Montero Dorta, Antonio D.
Angulo, Raul E.
Artale, Maria Celeste
Merchan, Manuel Enrique
author_role author
author2 Montero Dorta, Antonio D.
Angulo, Raul E.
Artale, Maria Celeste
Merchan, Manuel Enrique
author2_role author
author
author
author
dc.subject.none.fl_str_mv LARGE-SCALE STRUCTURE OF UNIVERSE
GALAXIES: STATISTICS
GALAXIES: GROUPS
GALAXIES: HALOES
topic LARGE-SCALE STRUCTURE OF UNIVERSE
GALAXIES: STATISTICS
GALAXIES: GROUPS
GALAXIES: HALOES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez & Merchán in order to determine the stellar and halo mass-size relations of central and satellite galaxies separately. We show that, while central and satellite galaxies display similar stellar mass-size relations, their halo mass-size relations differ significantly. As expected, more massive haloes tend to host larger central galaxies. However, the size of satellite galaxies depends only slightly on halo virial mass. We show that these results are compatible with a remarkably simple model in which the size of central and satellite galaxies scales as the cubic root of their host halo mass, with the normalization for satellites being ∼30 per cent smaller than that for central galaxies, which can be attributed to tidal stripping. We further check that our measurements are in excellent agreement with predictions from the IllustrisTNG hydrodynamical simulation. In the second part of this paper, we analyse how the clustering properties of central and satellite galaxies depend on their size. We demonstrate that, independently of the stellar mass threshold adopted, smaller galaxies are more tightly clustered than larger galaxies when either the entire sample or only satellites are considered. The opposite trend is observed on large scales when the size split is performed for the central galaxies alone. Our results place significant constraints for halo-galaxy connection models that link galaxy size with the properties of their hosting haloes.
Fil: Rodriguez, Facundo. 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: Montero Dorta, Antonio D.. Universidade de Sao Paulo; Brasil. Universidad Técnica Federico Santa María; Chile
Fil: Angulo, Raul E.. Ikerbasque, Basque Foundation For Science; España. Donostia International Physics Center; España
Fil: Artale, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Innsbruck; Austria
Fil: Merchan, Manuel Enrique. 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
description In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez & Merchán in order to determine the stellar and halo mass-size relations of central and satellite galaxies separately. We show that, while central and satellite galaxies display similar stellar mass-size relations, their halo mass-size relations differ significantly. As expected, more massive haloes tend to host larger central galaxies. However, the size of satellite galaxies depends only slightly on halo virial mass. We show that these results are compatible with a remarkably simple model in which the size of central and satellite galaxies scales as the cubic root of their host halo mass, with the normalization for satellites being ∼30 per cent smaller than that for central galaxies, which can be attributed to tidal stripping. We further check that our measurements are in excellent agreement with predictions from the IllustrisTNG hydrodynamical simulation. In the second part of this paper, we analyse how the clustering properties of central and satellite galaxies depend on their size. We demonstrate that, independently of the stellar mass threshold adopted, smaller galaxies are more tightly clustered than larger galaxies when either the entire sample or only satellites are considered. The opposite trend is observed on large scales when the size split is performed for the central galaxies alone. Our results place significant constraints for halo-galaxy connection models that link galaxy size with the properties of their hosting haloes.
publishDate 2021
dc.date.none.fl_str_mv 2021-08
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/11336/170944
Rodriguez, Facundo; Montero Dorta, Antonio D.; Angulo, Raul E.; Artale, Maria Celeste; Merchan, Manuel Enrique; The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 505; 3; 8-2021; 3192-3205
0035-8711
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/170944
identifier_str_mv Rodriguez, Facundo; Montero Dorta, Antonio D.; Angulo, Raul E.; Artale, Maria Celeste; Merchan, Manuel Enrique; The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 505; 3; 8-2021; 3192-3205
0035-8711
1365-2966
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab1571/6289926
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab1571
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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