Clustering properties of g-selected galaxies at z ~ 0.8

Autores
Favole, Ginevra; Comparat, Johan; Prada, Francisco; Yepes, Gustavo; Jullo, Eric; Niemiec, Anna; Kneib, Jean-Paul; Rodriguez Torres, Sergio A.; Klypin, Anatoly; Skibba, Ramin A.; McBride, Cameron K.; Eisenstein, Daniel J.; Schlegel, David J.; Nuza, Sebastian Ernesto; Chuang, Chia-Hsun; Delubac, Timotheé; Yèche, Christophe; Schneider, Donald P.; Schneider, Donald P.
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will use emission-line galaxies (ELGs) to probe cosmological models by mapping the large-scale structure of the Universe in the redshift range 0.6 < z < 1.7. With current data, we explore the halo-galaxy connection by measuring three clustering properties of g-selected ELGs as matter tracers in the redshift range 0.6 < z < 1: (i) the redshift-space two-point correlation function using spectroscopic redshifts from the BOSS ELG sample and VIPERS; (ii) the angular two-point correlation function on the footprint of the CFHT-LS; (iii) the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. We interpret these observations by mapping them on to the latest high-resolution MultiDark Planck N-body simulation, using a novel (Sub)Halo-Abundance Matching technique that accounts for the ELG incompleteness. ELGs at z ~ 0.8 live in haloes of (1 ± 0.5) × 10 12 h -1 M⊙ and 22.5 ± 2.5 per cent of them are satellites belonging to a larger halo. The halo occupation distribution of ELGs indicates that we are sampling the galaxies in which stars form in the most efficient way, according to their stellar-to-halo mass ratio.
Fil: Favole, Ginevra. Instituto de Fisica Teorica de Madrid; España
Fil: Comparat, Johan. Universidad Autónoma de Madrid; España
Fil: Prada, Francisco. Lawrence Berkeley National Laboratory; Estados Unidos. Universidad Autónoma de Madrid; España
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España
Fil: Jullo, Eric. Laboratoire D'astrophysique de Marseille; Francia
Fil: Niemiec, Anna. Laboratoire D'astrophysique de Marseille; Francia
Fil: Kneib, Jean-Paul. Laboratoire D'astrophysique de Marseille; Francia
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España
Fil: Klypin, Anatoly. New Mexico State University Las Cruces; México
Fil: Skibba, Ramin A.. University of California at San Diego; Estados Unidos
Fil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Nuza, Sebastian Ernesto. 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
Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; España
Fil: Delubac, Timotheé. Swiss Federal Institute Of Technology Epfl, Lausanne; Suiza
Fil: Yèche, Christophe. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia
Fil: Schneider, Donald P.. Pennsylvania State University;
Fil: Schneider, Donald P.. State University of Pennsylvania; Estados Unidos
Materia
COSMOLOGY: OBSERVATIONS - COSMOLOGY
GALAXIES: DISTANCES AND REDSHIFTS
GALAXIES: HALOES
GALAXIES: STATISTICS
THEORY - LARGE-SCALE STRUCTURE OF UNIVERSE
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:11336/76871
Acceder
id CONICETDig_d6cd15ac396a745dc6898761f9fb4977
oai_identifier_str oai:ri.conicet.gov.ar:11336/76871
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Clustering properties of g-selected galaxies at z ~ 0.8Favole, GinevraComparat, JohanPrada, FranciscoYepes, GustavoJullo, EricNiemiec, AnnaKneib, Jean-PaulRodriguez Torres, Sergio A.Klypin, AnatolySkibba, Ramin A.McBride, Cameron K.Eisenstein, Daniel J.Schlegel, David J.Nuza, Sebastian ErnestoChuang, Chia-HsunDelubac, TimotheéYèche, ChristopheSchneider, Donald P.Schneider, Donald P.COSMOLOGY: OBSERVATIONS - COSMOLOGYGALAXIES: DISTANCES AND REDSHIFTSGALAXIES: HALOESGALAXIES: STATISTICSTHEORY - LARGE-SCALE STRUCTURE OF UNIVERSEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will use emission-line galaxies (ELGs) to probe cosmological models by mapping the large-scale structure of the Universe in the redshift range 0.6 < z < 1.7. With current data, we explore the halo-galaxy connection by measuring three clustering properties of g-selected ELGs as matter tracers in the redshift range 0.6 < z < 1: (i) the redshift-space two-point correlation function using spectroscopic redshifts from the BOSS ELG sample and VIPERS; (ii) the angular two-point correlation function on the footprint of the CFHT-LS; (iii) the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. We interpret these observations by mapping them on to the latest high-resolution MultiDark Planck N-body simulation, using a novel (Sub)Halo-Abundance Matching technique that accounts for the ELG incompleteness. ELGs at z ~ 0.8 live in haloes of (1 ± 0.5) × 10 12 h -1 M⊙ and 22.5 ± 2.5 per cent of them are satellites belonging to a larger halo. The halo occupation distribution of ELGs indicates that we are sampling the galaxies in which stars form in the most efficient way, according to their stellar-to-halo mass ratio.Fil: Favole, Ginevra. Instituto de Fisica Teorica de Madrid; EspañaFil: Comparat, Johan. Universidad Autónoma de Madrid; EspañaFil: Prada, Francisco. Lawrence Berkeley National Laboratory; Estados Unidos. Universidad Autónoma de Madrid; EspañaFil: Yepes, Gustavo. Universidad Autónoma de Madrid; EspañaFil: Jullo, Eric. Laboratoire D'astrophysique de Marseille; FranciaFil: Niemiec, Anna. Laboratoire D'astrophysique de Marseille; FranciaFil: Kneib, Jean-Paul. Laboratoire D'astrophysique de Marseille; FranciaFil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; EspañaFil: Klypin, Anatoly. New Mexico State University Las Cruces; MéxicoFil: Skibba, Ramin A.. University of California at San Diego; Estados UnidosFil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Nuza, Sebastian Ernesto. 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; ArgentinaFil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; EspañaFil: Delubac, Timotheé. Swiss Federal Institute Of Technology Epfl, Lausanne; SuizaFil: Yèche, Christophe. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; FranciaFil: Schneider, Donald P.. Pennsylvania State University;Fil: Schneider, Donald P.. State University of Pennsylvania; Estados UnidosWiley Blackwell Publishing, Inc2016-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/76871Favole, Ginevra; Comparat, Johan; Prada, Francisco; Yepes, Gustavo; Jullo, Eric; et al.; Clustering properties of g-selected galaxies at z ~ 0.8; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 4; 10-2016; 3421-34310035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw1483info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:42:30Zoai:ri.conicet.gov.ar:11336/76871instacron: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 09:42:31.219CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Clustering properties of g-selected galaxies at z ~ 0.8
title Clustering properties of g-selected galaxies at z ~ 0.8
spellingShingle Clustering properties of g-selected galaxies at z ~ 0.8
Favole, Ginevra
COSMOLOGY: OBSERVATIONS - COSMOLOGY
GALAXIES: DISTANCES AND REDSHIFTS
GALAXIES: HALOES
GALAXIES: STATISTICS
THEORY - LARGE-SCALE STRUCTURE OF UNIVERSE
title_short Clustering properties of g-selected galaxies at z ~ 0.8
title_full Clustering properties of g-selected galaxies at z ~ 0.8
title_fullStr Clustering properties of g-selected galaxies at z ~ 0.8
title_full_unstemmed Clustering properties of g-selected galaxies at z ~ 0.8
title_sort Clustering properties of g-selected galaxies at z ~ 0.8
dc.creator.none.fl_str_mv Favole, Ginevra
Comparat, Johan
Prada, Francisco
Yepes, Gustavo
Jullo, Eric
Niemiec, Anna
Kneib, Jean-Paul
Rodriguez Torres, Sergio A.
Klypin, Anatoly
Skibba, Ramin A.
McBride, Cameron K.
Eisenstein, Daniel J.
Schlegel, David J.
Nuza, Sebastian Ernesto
Chuang, Chia-Hsun
Delubac, Timotheé
Yèche, Christophe
Schneider, Donald P.
Schneider, Donald P.
author Favole, Ginevra
author_facet Favole, Ginevra
Comparat, Johan
Prada, Francisco
Yepes, Gustavo
Jullo, Eric
Niemiec, Anna
Kneib, Jean-Paul
Rodriguez Torres, Sergio A.
Klypin, Anatoly
Skibba, Ramin A.
McBride, Cameron K.
Eisenstein, Daniel J.
Schlegel, David J.
Nuza, Sebastian Ernesto
Chuang, Chia-Hsun
Delubac, Timotheé
Yèche, Christophe
Schneider, Donald P.
author_role author
author2 Comparat, Johan
Prada, Francisco
Yepes, Gustavo
Jullo, Eric
Niemiec, Anna
Kneib, Jean-Paul
Rodriguez Torres, Sergio A.
Klypin, Anatoly
Skibba, Ramin A.
McBride, Cameron K.
Eisenstein, Daniel J.
Schlegel, David J.
Nuza, Sebastian Ernesto
Chuang, Chia-Hsun
Delubac, Timotheé
Yèche, Christophe
Schneider, Donald P.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv COSMOLOGY: OBSERVATIONS - COSMOLOGY
GALAXIES: DISTANCES AND REDSHIFTS
GALAXIES: HALOES
GALAXIES: STATISTICS
THEORY - LARGE-SCALE STRUCTURE OF UNIVERSE
topic COSMOLOGY: OBSERVATIONS - COSMOLOGY
GALAXIES: DISTANCES AND REDSHIFTS
GALAXIES: HALOES
GALAXIES: STATISTICS
THEORY - LARGE-SCALE STRUCTURE OF UNIVERSE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will use emission-line galaxies (ELGs) to probe cosmological models by mapping the large-scale structure of the Universe in the redshift range 0.6 < z < 1.7. With current data, we explore the halo-galaxy connection by measuring three clustering properties of g-selected ELGs as matter tracers in the redshift range 0.6 < z < 1: (i) the redshift-space two-point correlation function using spectroscopic redshifts from the BOSS ELG sample and VIPERS; (ii) the angular two-point correlation function on the footprint of the CFHT-LS; (iii) the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. We interpret these observations by mapping them on to the latest high-resolution MultiDark Planck N-body simulation, using a novel (Sub)Halo-Abundance Matching technique that accounts for the ELG incompleteness. ELGs at z ~ 0.8 live in haloes of (1 ± 0.5) × 10 12 h -1 M⊙ and 22.5 ± 2.5 per cent of them are satellites belonging to a larger halo. The halo occupation distribution of ELGs indicates that we are sampling the galaxies in which stars form in the most efficient way, according to their stellar-to-halo mass ratio.
Fil: Favole, Ginevra. Instituto de Fisica Teorica de Madrid; España
Fil: Comparat, Johan. Universidad Autónoma de Madrid; España
Fil: Prada, Francisco. Lawrence Berkeley National Laboratory; Estados Unidos. Universidad Autónoma de Madrid; España
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España
Fil: Jullo, Eric. Laboratoire D'astrophysique de Marseille; Francia
Fil: Niemiec, Anna. Laboratoire D'astrophysique de Marseille; Francia
Fil: Kneib, Jean-Paul. Laboratoire D'astrophysique de Marseille; Francia
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España
Fil: Klypin, Anatoly. New Mexico State University Las Cruces; México
Fil: Skibba, Ramin A.. University of California at San Diego; Estados Unidos
Fil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Nuza, Sebastian Ernesto. 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
Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; España
Fil: Delubac, Timotheé. Swiss Federal Institute Of Technology Epfl, Lausanne; Suiza
Fil: Yèche, Christophe. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia
Fil: Schneider, Donald P.. Pennsylvania State University;
Fil: Schneider, Donald P.. State University of Pennsylvania; Estados Unidos
description Current and future large redshift surveys, as the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (SDSS-IV/eBOSS) or the Dark Energy Spectroscopic Instrument (DESI), will use emission-line galaxies (ELGs) to probe cosmological models by mapping the large-scale structure of the Universe in the redshift range 0.6 < z < 1.7. With current data, we explore the halo-galaxy connection by measuring three clustering properties of g-selected ELGs as matter tracers in the redshift range 0.6 < z < 1: (i) the redshift-space two-point correlation function using spectroscopic redshifts from the BOSS ELG sample and VIPERS; (ii) the angular two-point correlation function on the footprint of the CFHT-LS; (iii) the galaxy-galaxy lensing signal around the ELGs using the CFHTLenS. We interpret these observations by mapping them on to the latest high-resolution MultiDark Planck N-body simulation, using a novel (Sub)Halo-Abundance Matching technique that accounts for the ELG incompleteness. ELGs at z ~ 0.8 live in haloes of (1 ± 0.5) × 10 12 h -1 M⊙ and 22.5 ± 2.5 per cent of them are satellites belonging to a larger halo. The halo occupation distribution of ELGs indicates that we are sampling the galaxies in which stars form in the most efficient way, according to their stellar-to-halo mass ratio.
publishDate 2016
dc.date.none.fl_str_mv 2016-10
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/11336/76871
Favole, Ginevra; Comparat, Johan; Prada, Francisco; Yepes, Gustavo; Jullo, Eric; et al.; Clustering properties of g-selected galaxies at z ~ 0.8; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 4; 10-2016; 3421-3431
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/76871
identifier_str_mv Favole, Ginevra; Comparat, Johan; Prada, Francisco; Yepes, Gustavo; Jullo, Eric; et al.; Clustering properties of g-selected galaxies at z ~ 0.8; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 4; 10-2016; 3421-3431
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/doi/10.1093/mnras/stw1483
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 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
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
_version_ 1844613339396702208
score 13.070432

Publicaciones similares