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dc.contributor.author
Favole, Ginevra
dc.contributor.author
Comparat, Johan
dc.contributor.author
Prada, Francisco
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Yepes, Gustavo
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Jullo, Eric
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Niemiec, Anna
dc.contributor.author
Kneib, Jean-Paul
dc.contributor.author
Rodriguez Torres, Sergio A.
dc.contributor.author
Klypin, Anatoly
dc.contributor.author
Skibba, Ramin A.
dc.contributor.author
McBride, Cameron K.
dc.contributor.author
Eisenstein, Daniel J.
dc.contributor.author
Schlegel, David J.
dc.contributor.author
Nuza, Sebastian Ernesto
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Chuang, Chia-Hsun
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Delubac, Timotheé
dc.contributor.author
Yèche, Christophe
dc.contributor.author
Schneider, Donald P.
dc.contributor.author
Schneider, Donald P.
dc.date.available
2019-05-22T17:32:47Z
dc.date.issued
2016-10
dc.identifier.citation
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
dc.identifier.issn
0035-8711
dc.identifier.uri
http://hdl.handle.net/11336/76871
dc.description.abstract
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.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Wiley Blackwell Publishing, Inc
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Cosmology: Observations - Cosmology
dc.subject
Galaxies: Distances And Redshifts
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Galaxies: Haloes
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Galaxies: Statistics
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Theory - Large-Scale Structure of Universe
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Clustering properties of g-selected galaxies at z ~ 0.8
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2019-05-14T21:37:17Z
dc.journal.volume
461
dc.journal.number
4
dc.journal.pagination
3421-3431
dc.journal.pais
Reino Unido
dc.journal.ciudad
Londres
dc.description.fil
Fil: Favole, Ginevra. Instituto de Fisica Teorica de Madrid; España
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Fil: Comparat, Johan. Universidad Autónoma de Madrid; España
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Fil: Prada, Francisco. Lawrence Berkeley National Laboratory; Estados Unidos. Universidad Autónoma de Madrid; España
dc.description.fil
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España
dc.description.fil
Fil: Jullo, Eric. Laboratoire D'astrophysique de Marseille; Francia
dc.description.fil
Fil: Niemiec, Anna. Laboratoire D'astrophysique de Marseille; Francia
dc.description.fil
Fil: Kneib, Jean-Paul. Laboratoire D'astrophysique de Marseille; Francia
dc.description.fil
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España
dc.description.fil
Fil: Klypin, Anatoly. New Mexico State University Las Cruces; México
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Fil: Skibba, Ramin A.. University of California at San Diego; Estados Unidos
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Fil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
dc.description.fil
Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
dc.description.fil
Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos
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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
dc.description.fil
Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; España
dc.description.fil
Fil: Delubac, Timotheé. Swiss Federal Institute Of Technology Epfl, Lausanne; Suiza
dc.description.fil
Fil: Yèche, Christophe. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia
dc.description.fil
Fil: Schneider, Donald P.. Pennsylvania State University;
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Fil: Schneider, Donald P.. State University of Pennsylvania; Estados Unidos
dc.journal.title
Monthly Notices of the Royal Astronomical Society
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stw1483
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