ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure
- Autores
- Ramakrishnan, Vandana; Moon, Byeongha; Im, Sang Hyeok; Farooq, Rameen; Lee, Kyoung Soo; Gawiser, Eric; Yang, Yujin; Park, Changbom; Hwang, Ho Seong; Valdes, Francisco; Artale, Maria Celeste; Ciardullo, Robin; Dey, Arjun; Gronwall, Caryl; Guaita, Lucia; Jeong, Woong Seob; Padilla, Nelson David; Singh, Akriti; Zabludoff, Ann
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- While many Lyα blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Lyα emitters (LAEs) and 129 LABs at z = 3.1 identified over a ∼9.5 deg2 area in early data from the ongoing One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey to investigate this question. Using LAEs as tracers of the underlying matter distribution, we identify overdense structures as galaxy groups, protoclusters, and filaments of the cosmic web. We find that LABs preferentially reside in regions of higher-than-average density and are located in closer proximity to overdense structures, which represent the sites of protoclusters and their substructures. Moreover, protoclusters hosting one or more LABs tend to have a higher descendant mass than those which do not. Blobs are also strongly associated with filaments of the cosmic web, with ∼70% of the population being within a projected distance of ∼2.4 pMpc from a filament. We show that the proximity of LABs to protoclusters is naturally explained by their association with filaments as large cosmic structures are where many filaments converge. The contiguous wide-field coverage of the ODIN survey allows us to establish firmly a connection between LABs as a population and filaments of the cosmic web for the first time.
Fil: Ramakrishnan, Vandana. Purdue University; Estados Unidos
Fil: Moon, Byeongha. Korea Astronomy And Space Science Institute; Corea del Norte
Fil: Im, Sang Hyeok. Seoul National University; Corea del Norte
Fil: Farooq, Rameen. Rutgers Universitynew Brunswick; Estados Unidos
Fil: Lee, Kyoung Soo. Purdue University; Estados Unidos
Fil: Gawiser, Eric. Rutgers Universitynew Brunswick; Estados Unidos
Fil: Yang, Yujin. Korea Astronomy And Space Science Institute; Corea del Norte
Fil: Park, Changbom. Korea Institute For Advanced Study; Corea del Norte
Fil: Hwang, Ho Seong. Seoul National University; Corea del Norte
Fil: Valdes, Francisco. National Optical Astronomy Observatory; Estados Unidos
Fil: Artale, Maria Celeste. Universidad Andrés Bello; Chile. Università di Padova; Italia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Purdue University; Estados Unidos
Fil: Ciardullo, Robin. University of Pennsylvania; Estados Unidos
Fil: Dey, Arjun. No especifíca;
Fil: Gronwall, Caryl. University of Pennsylvania; Estados Unidos
Fil: Guaita, Lucia. Universidad Andrés Bello; Chile
Fil: Jeong, Woong Seob. Korea Astronomy And Space Science Institute; Corea del Norte
Fil: Padilla, Nelson David. 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: Singh, Akriti. Universidad Andrés Bello; Chile
Fil: Zabludoff, Ann. University of Arizona; Estados Unidos - Materia
-
high-redshift galaxies
galaxy clusters
lyman-alpha galaxies - 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:11336/231628
Ver los metadatos del registro completo
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ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale StructureRamakrishnan, VandanaMoon, ByeonghaIm, Sang HyeokFarooq, RameenLee, Kyoung SooGawiser, EricYang, YujinPark, ChangbomHwang, Ho SeongValdes, FranciscoArtale, Maria CelesteCiardullo, RobinDey, ArjunGronwall, CarylGuaita, LuciaJeong, Woong SeobPadilla, Nelson DavidSingh, AkritiZabludoff, Annhigh-redshift galaxiesgalaxy clusterslyman-alpha galaxieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1While many Lyα blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Lyα emitters (LAEs) and 129 LABs at z = 3.1 identified over a ∼9.5 deg2 area in early data from the ongoing One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey to investigate this question. Using LAEs as tracers of the underlying matter distribution, we identify overdense structures as galaxy groups, protoclusters, and filaments of the cosmic web. We find that LABs preferentially reside in regions of higher-than-average density and are located in closer proximity to overdense structures, which represent the sites of protoclusters and their substructures. Moreover, protoclusters hosting one or more LABs tend to have a higher descendant mass than those which do not. Blobs are also strongly associated with filaments of the cosmic web, with ∼70% of the population being within a projected distance of ∼2.4 pMpc from a filament. We show that the proximity of LABs to protoclusters is naturally explained by their association with filaments as large cosmic structures are where many filaments converge. The contiguous wide-field coverage of the ODIN survey allows us to establish firmly a connection between LABs as a population and filaments of the cosmic web for the first time.Fil: Ramakrishnan, Vandana. Purdue University; Estados UnidosFil: Moon, Byeongha. Korea Astronomy And Space Science Institute; Corea del NorteFil: Im, Sang Hyeok. Seoul National University; Corea del NorteFil: Farooq, Rameen. Rutgers Universitynew Brunswick; Estados UnidosFil: Lee, Kyoung Soo. Purdue University; Estados UnidosFil: Gawiser, Eric. Rutgers Universitynew Brunswick; Estados UnidosFil: Yang, Yujin. Korea Astronomy And Space Science Institute; Corea del NorteFil: Park, Changbom. Korea Institute For Advanced Study; Corea del NorteFil: Hwang, Ho Seong. Seoul National University; Corea del NorteFil: Valdes, Francisco. National Optical Astronomy Observatory; Estados UnidosFil: Artale, Maria Celeste. Universidad Andrés Bello; Chile. Università di Padova; Italia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Purdue University; Estados UnidosFil: Ciardullo, Robin. University of Pennsylvania; Estados UnidosFil: Dey, Arjun. No especifíca;Fil: Gronwall, Caryl. University of Pennsylvania; Estados UnidosFil: Guaita, Lucia. Universidad Andrés Bello; ChileFil: Jeong, Woong Seob. Korea Astronomy And Space Science Institute; Corea del NorteFil: Padilla, Nelson David. 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: Singh, Akriti. Universidad Andrés Bello; ChileFil: Zabludoff, Ann. University of Arizona; Estados UnidosIOP Publishing2023-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/231628Ramakrishnan, Vandana; Moon, Byeongha; Im, Sang Hyeok; Farooq, Rameen; Lee, Kyoung Soo; et al.; ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure; IOP Publishing; Astrophysical Journal; 951; 2; 7-2023; 1-200004-637X1538-4357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/acd341info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:06Zoai:ri.conicet.gov.ar:11336/231628instacron: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 10:04:06.877CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
title |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
spellingShingle |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure Ramakrishnan, Vandana high-redshift galaxies galaxy clusters lyman-alpha galaxies |
title_short |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
title_full |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
title_fullStr |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
title_full_unstemmed |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
title_sort |
ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure |
dc.creator.none.fl_str_mv |
Ramakrishnan, Vandana Moon, Byeongha Im, Sang Hyeok Farooq, Rameen Lee, Kyoung Soo Gawiser, Eric Yang, Yujin Park, Changbom Hwang, Ho Seong Valdes, Francisco Artale, Maria Celeste Ciardullo, Robin Dey, Arjun Gronwall, Caryl Guaita, Lucia Jeong, Woong Seob Padilla, Nelson David Singh, Akriti Zabludoff, Ann |
author |
Ramakrishnan, Vandana |
author_facet |
Ramakrishnan, Vandana Moon, Byeongha Im, Sang Hyeok Farooq, Rameen Lee, Kyoung Soo Gawiser, Eric Yang, Yujin Park, Changbom Hwang, Ho Seong Valdes, Francisco Artale, Maria Celeste Ciardullo, Robin Dey, Arjun Gronwall, Caryl Guaita, Lucia Jeong, Woong Seob Padilla, Nelson David Singh, Akriti Zabludoff, Ann |
author_role |
author |
author2 |
Moon, Byeongha Im, Sang Hyeok Farooq, Rameen Lee, Kyoung Soo Gawiser, Eric Yang, Yujin Park, Changbom Hwang, Ho Seong Valdes, Francisco Artale, Maria Celeste Ciardullo, Robin Dey, Arjun Gronwall, Caryl Guaita, Lucia Jeong, Woong Seob Padilla, Nelson David Singh, Akriti Zabludoff, Ann |
author2_role |
author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
high-redshift galaxies galaxy clusters lyman-alpha galaxies |
topic |
high-redshift galaxies galaxy clusters lyman-alpha galaxies |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
While many Lyα blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Lyα emitters (LAEs) and 129 LABs at z = 3.1 identified over a ∼9.5 deg2 area in early data from the ongoing One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey to investigate this question. Using LAEs as tracers of the underlying matter distribution, we identify overdense structures as galaxy groups, protoclusters, and filaments of the cosmic web. We find that LABs preferentially reside in regions of higher-than-average density and are located in closer proximity to overdense structures, which represent the sites of protoclusters and their substructures. Moreover, protoclusters hosting one or more LABs tend to have a higher descendant mass than those which do not. Blobs are also strongly associated with filaments of the cosmic web, with ∼70% of the population being within a projected distance of ∼2.4 pMpc from a filament. We show that the proximity of LABs to protoclusters is naturally explained by their association with filaments as large cosmic structures are where many filaments converge. The contiguous wide-field coverage of the ODIN survey allows us to establish firmly a connection between LABs as a population and filaments of the cosmic web for the first time. Fil: Ramakrishnan, Vandana. Purdue University; Estados Unidos Fil: Moon, Byeongha. Korea Astronomy And Space Science Institute; Corea del Norte Fil: Im, Sang Hyeok. Seoul National University; Corea del Norte Fil: Farooq, Rameen. Rutgers Universitynew Brunswick; Estados Unidos Fil: Lee, Kyoung Soo. Purdue University; Estados Unidos Fil: Gawiser, Eric. Rutgers Universitynew Brunswick; Estados Unidos Fil: Yang, Yujin. Korea Astronomy And Space Science Institute; Corea del Norte Fil: Park, Changbom. Korea Institute For Advanced Study; Corea del Norte Fil: Hwang, Ho Seong. Seoul National University; Corea del Norte Fil: Valdes, Francisco. National Optical Astronomy Observatory; Estados Unidos Fil: Artale, Maria Celeste. Universidad Andrés Bello; Chile. Università di Padova; Italia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Purdue University; Estados Unidos Fil: Ciardullo, Robin. University of Pennsylvania; Estados Unidos Fil: Dey, Arjun. No especifíca; Fil: Gronwall, Caryl. University of Pennsylvania; Estados Unidos Fil: Guaita, Lucia. Universidad Andrés Bello; Chile Fil: Jeong, Woong Seob. Korea Astronomy And Space Science Institute; Corea del Norte Fil: Padilla, Nelson David. 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: Singh, Akriti. Universidad Andrés Bello; Chile Fil: Zabludoff, Ann. University of Arizona; Estados Unidos |
description |
While many Lyα blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Lyα emitters (LAEs) and 129 LABs at z = 3.1 identified over a ∼9.5 deg2 area in early data from the ongoing One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey to investigate this question. Using LAEs as tracers of the underlying matter distribution, we identify overdense structures as galaxy groups, protoclusters, and filaments of the cosmic web. We find that LABs preferentially reside in regions of higher-than-average density and are located in closer proximity to overdense structures, which represent the sites of protoclusters and their substructures. Moreover, protoclusters hosting one or more LABs tend to have a higher descendant mass than those which do not. Blobs are also strongly associated with filaments of the cosmic web, with ∼70% of the population being within a projected distance of ∼2.4 pMpc from a filament. We show that the proximity of LABs to protoclusters is naturally explained by their association with filaments as large cosmic structures are where many filaments converge. The contiguous wide-field coverage of the ODIN survey allows us to establish firmly a connection between LABs as a population and filaments of the cosmic web for the first time. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-07 |
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/11336/231628 Ramakrishnan, Vandana; Moon, Byeongha; Im, Sang Hyeok; Farooq, Rameen; Lee, Kyoung Soo; et al.; ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure; IOP Publishing; Astrophysical Journal; 951; 2; 7-2023; 1-20 0004-637X 1538-4357 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/231628 |
identifier_str_mv |
Ramakrishnan, Vandana; Moon, Byeongha; Im, Sang Hyeok; Farooq, Rameen; Lee, Kyoung Soo; et al.; ODIN: Where Do Lyα Blobs Live?: Contextualizing Blob Environments within Large-scale Structure; IOP Publishing; Astrophysical Journal; 951; 2; 7-2023; 1-20 0004-637X 1538-4357 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/acd341 |
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 |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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1844613864716500992 |
score |
13.070432 |