Are Ly α emitters segregated in protoclusters regions?
- Autores
- Hough, Tomas; Gurung López, Siddhartha; Orsi, Álvaro; Cora, Sofia Alejandra; Lacey, Cedric G; Baugh, Carlton M
- Año de publicación
- 2020
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The presence of neutral hydrogen in the interstellar medium (ISM) and intergalactic medium (IGM) induces radiative transfer (RT) effects on LyαLyα photons that affect the observability of Lyman alpha emitters (LAEs). We use the GALFORM semi-analytic model of galaxy formation and evolution to analyse how these effects shape the spatial distribution of LAEs with respect to HαHα emitters (HAEs) around high-density regions at high redshift. We find that when a large sample of protoclusters is considered, HAEs showing also LyαLyα emission (HAEs + LAEs) populate the same regions as those that do not display the LyαLyα line at zz = 2.2. We compare against the protocluster USS1558-003, one of the most massive protoclusters located at zz = 2.53. Our results indicate that the strong depletion of HAEs + LAEs present in the high-density regions of USS1558-003 may be due to cosmic variance. We find that at zz = 2.2 and zz = 3.0, RT of the ISM produces a strong decline (30-50 per cent) of the clustering amplitude of HAEs + LAEs with respect to HAEs towards the protoclusters centre. At zz = 5.7, given the early evolutionary state of protoclusters and galaxies, the clustering of HAEs + LAEs has a smaller variation (10-20 per cent) towards the protoclusters centre. Depending on the equivalent width and luminosity criteria of the emission-line galaxy sample, the IGM can have a mild or a null effect on galaxy properties and clustering in high-density regions.
Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Gurung López, Siddhartha. Department Of Physics, Missouri University Of Science; Estados Unidos
Fil: Orsi, Álvaro. Centro de Estudios de Física del Cosmos de Aragón; España
Fil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Lacey, Cedric G. Institute For Computational Cosmology; Reino Unido
Fil: Baugh, Carlton M. Institute For Computational Cosmology; Reino Unido - Materia
-
Radiative transfer
methods: numerical
Galaxies: clusters: general
Galaxies: high-redshift
Galaxies: clusters: intracluster medium - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/142044
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Are Ly α emitters segregated in protoclusters regions?Hough, TomasGurung López, SiddharthaOrsi, ÁlvaroCora, Sofia AlejandraLacey, Cedric GBaugh, Carlton MRadiative transfermethods: numericalGalaxies: clusters: generalGalaxies: high-redshiftGalaxies: clusters: intracluster mediumhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The presence of neutral hydrogen in the interstellar medium (ISM) and intergalactic medium (IGM) induces radiative transfer (RT) effects on LyαLyα photons that affect the observability of Lyman alpha emitters (LAEs). We use the GALFORM semi-analytic model of galaxy formation and evolution to analyse how these effects shape the spatial distribution of LAEs with respect to HαHα emitters (HAEs) around high-density regions at high redshift. We find that when a large sample of protoclusters is considered, HAEs showing also LyαLyα emission (HAEs + LAEs) populate the same regions as those that do not display the LyαLyα line at zz = 2.2. We compare against the protocluster USS1558-003, one of the most massive protoclusters located at zz = 2.53. Our results indicate that the strong depletion of HAEs + LAEs present in the high-density regions of USS1558-003 may be due to cosmic variance. We find that at zz = 2.2 and zz = 3.0, RT of the ISM produces a strong decline (30-50 per cent) of the clustering amplitude of HAEs + LAEs with respect to HAEs towards the protoclusters centre. At zz = 5.7, given the early evolutionary state of protoclusters and galaxies, the clustering of HAEs + LAEs has a smaller variation (10-20 per cent) towards the protoclusters centre. Depending on the equivalent width and luminosity criteria of the emission-line galaxy sample, the IGM can have a mild or a null effect on galaxy properties and clustering in high-density regions.Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Gurung López, Siddhartha. Department Of Physics, Missouri University Of Science; Estados UnidosFil: Orsi, Álvaro. Centro de Estudios de Física del Cosmos de Aragón; EspañaFil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Lacey, Cedric G. Institute For Computational Cosmology; Reino UnidoFil: Baugh, Carlton M. Institute For Computational Cosmology; Reino UnidoWiley Blackwell Publishing, Inc2020-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/142044Hough, Tomas; Gurung López, Siddhartha; Orsi, Álvaro; Cora, Sofia Alejandra; Lacey, Cedric G; et al.; Are Ly α emitters segregated in protoclusters regions?; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 499; 2; 12-2020; 2104-21150035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/499/2/2104/5917099info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:11:17Zoai:ri.conicet.gov.ar:11336/142044instacron: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 10:11:17.847CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Are Ly α emitters segregated in protoclusters regions? |
title |
Are Ly α emitters segregated in protoclusters regions? |
spellingShingle |
Are Ly α emitters segregated in protoclusters regions? Hough, Tomas Radiative transfer methods: numerical Galaxies: clusters: general Galaxies: high-redshift Galaxies: clusters: intracluster medium |
title_short |
Are Ly α emitters segregated in protoclusters regions? |
title_full |
Are Ly α emitters segregated in protoclusters regions? |
title_fullStr |
Are Ly α emitters segregated in protoclusters regions? |
title_full_unstemmed |
Are Ly α emitters segregated in protoclusters regions? |
title_sort |
Are Ly α emitters segregated in protoclusters regions? |
dc.creator.none.fl_str_mv |
Hough, Tomas Gurung López, Siddhartha Orsi, Álvaro Cora, Sofia Alejandra Lacey, Cedric G Baugh, Carlton M |
author |
Hough, Tomas |
author_facet |
Hough, Tomas Gurung López, Siddhartha Orsi, Álvaro Cora, Sofia Alejandra Lacey, Cedric G Baugh, Carlton M |
author_role |
author |
author2 |
Gurung López, Siddhartha Orsi, Álvaro Cora, Sofia Alejandra Lacey, Cedric G Baugh, Carlton M |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Radiative transfer methods: numerical Galaxies: clusters: general Galaxies: high-redshift Galaxies: clusters: intracluster medium |
topic |
Radiative transfer methods: numerical Galaxies: clusters: general Galaxies: high-redshift Galaxies: clusters: intracluster medium |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The presence of neutral hydrogen in the interstellar medium (ISM) and intergalactic medium (IGM) induces radiative transfer (RT) effects on LyαLyα photons that affect the observability of Lyman alpha emitters (LAEs). We use the GALFORM semi-analytic model of galaxy formation and evolution to analyse how these effects shape the spatial distribution of LAEs with respect to HαHα emitters (HAEs) around high-density regions at high redshift. We find that when a large sample of protoclusters is considered, HAEs showing also LyαLyα emission (HAEs + LAEs) populate the same regions as those that do not display the LyαLyα line at zz = 2.2. We compare against the protocluster USS1558-003, one of the most massive protoclusters located at zz = 2.53. Our results indicate that the strong depletion of HAEs + LAEs present in the high-density regions of USS1558-003 may be due to cosmic variance. We find that at zz = 2.2 and zz = 3.0, RT of the ISM produces a strong decline (30-50 per cent) of the clustering amplitude of HAEs + LAEs with respect to HAEs towards the protoclusters centre. At zz = 5.7, given the early evolutionary state of protoclusters and galaxies, the clustering of HAEs + LAEs has a smaller variation (10-20 per cent) towards the protoclusters centre. Depending on the equivalent width and luminosity criteria of the emission-line galaxy sample, the IGM can have a mild or a null effect on galaxy properties and clustering in high-density regions. Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Gurung López, Siddhartha. Department Of Physics, Missouri University Of Science; Estados Unidos Fil: Orsi, Álvaro. Centro de Estudios de Física del Cosmos de Aragón; España Fil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Lacey, Cedric G. Institute For Computational Cosmology; Reino Unido Fil: Baugh, Carlton M. Institute For Computational Cosmology; Reino Unido |
description |
The presence of neutral hydrogen in the interstellar medium (ISM) and intergalactic medium (IGM) induces radiative transfer (RT) effects on LyαLyα photons that affect the observability of Lyman alpha emitters (LAEs). We use the GALFORM semi-analytic model of galaxy formation and evolution to analyse how these effects shape the spatial distribution of LAEs with respect to HαHα emitters (HAEs) around high-density regions at high redshift. We find that when a large sample of protoclusters is considered, HAEs showing also LyαLyα emission (HAEs + LAEs) populate the same regions as those that do not display the LyαLyα line at zz = 2.2. We compare against the protocluster USS1558-003, one of the most massive protoclusters located at zz = 2.53. Our results indicate that the strong depletion of HAEs + LAEs present in the high-density regions of USS1558-003 may be due to cosmic variance. We find that at zz = 2.2 and zz = 3.0, RT of the ISM produces a strong decline (30-50 per cent) of the clustering amplitude of HAEs + LAEs with respect to HAEs towards the protoclusters centre. At zz = 5.7, given the early evolutionary state of protoclusters and galaxies, the clustering of HAEs + LAEs has a smaller variation (10-20 per cent) towards the protoclusters centre. Depending on the equivalent width and luminosity criteria of the emission-line galaxy sample, the IGM can have a mild or a null effect on galaxy properties and clustering in high-density regions. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-12 |
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/11336/142044 Hough, Tomas; Gurung López, Siddhartha; Orsi, Álvaro; Cora, Sofia Alejandra; Lacey, Cedric G; et al.; Are Ly α emitters segregated in protoclusters regions?; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 499; 2; 12-2020; 2104-2115 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/142044 |
identifier_str_mv |
Hough, Tomas; Gurung López, Siddhartha; Orsi, Álvaro; Cora, Sofia Alejandra; Lacey, Cedric G; et al.; Are Ly α emitters segregated in protoclusters regions?; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 499; 2; 12-2020; 2104-2115 0035-8711 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/article/499/2/2104/5917099 |
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 |
dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1844614010359513088 |
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13.070432 |