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http://hdl.handle.net/10261/150345
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dc.contributor.author | Favole, Ginevra | - |
dc.contributor.author | Comparat, Johan | - |
dc.contributor.author | Prada, Francisco | - |
dc.contributor.author | Schneider, D.P. | - |
dc.date.accessioned | 2017-05-24T12:23:33Z | - |
dc.date.available | 2017-05-24T12:23:33Z | - |
dc.date.issued | 2016 | - |
dc.identifier | doi: 10.1093/mnras/stw1483 | - |
dc.identifier | issn: 1365-2966 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society 461: 3421- 3431 (2016) | - |
dc.identifier.uri | http://hdl.handle.net/10261/150345 | - |
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 hM⊙ 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. © 2016 The Authors. | - |
dc.description.sponsorship | GF is supported by the Ministerio de Educacion y Ciencia of the Spanish Government through FPI grant AYA2010-2131-C02-01. JC acknowledges financial support from MINECO (Spain) under project number AYA2012-31101. GY acknowledges financial support from MINECO (Spain) under project number AYA2012-31101 and grant FPA2012-34694. EJ acknowledges the support of CNRS, and the Labex OCEVU. SEN acknowledges support by the Deutsche Forschungsgemeinschaft under the grant NU 332/21. GF, FP, SART, AK, SN and CC acknowledge financial support from the Spanish MICINN Consolider-Ingenio 2010 Programme under grant MultiDark CSD2009-00064, MINECO Centro de Excelencia Severo Ochoa Programme under grant SEV-2012-0249, and MINECO grant AYA2014-60641-C2-1-P. GF, JC and FP wish to thank the Lawrence Berkeley National Laboratory for the hospitality during the creation of this work. FP acknowledges the spanish MEC 'Salvador de Madariaga' program, Ref. PRX14/00444. | - |
dc.publisher | Oxford University Press | - |
dc.relation | info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2014-60641-C2-1-P | - |
dc.relation.isversionof | Publisher's version | - |
dc.rights | openAccess | - |
dc.subject | Galaxies: statistics | - |
dc.subject | Galaxies: haloes | - |
dc.subject | Galaxies: distances and redshifts | - |
dc.subject | Theory - large-scale structure of Universe | - |
dc.subject | Cosmology: observations - cosmology | - |
dc.title | Clustering properties of g-selected galaxies at z ~ 0.8 | - |
dc.type | artículo | - |
dc.identifier.doi | 10.1093/mnras/stw1483 | - |
dc.date.updated | 2017-05-24T12:23:34Z | - |
dc.description.version | Peer Reviewed | - |
dc.language.rfc3066 | eng | - |
dc.rights.license | http://dx.doi.org/10.1093/mnras/stw1483 | - |
dc.contributor.funder | German Research Foundation | - |
dc.contributor.funder | Centre National de la Recherche Scientifique (France) | - |
dc.contributor.funder | Ministerio de Economía y Competitividad (España) | - |
dc.contributor.funder | Ministerio de Educación y Ciencia (España) | - |
dc.contributor.funder | Ministerio de Ciencia e Innovación (España) | - |
dc.relation.csic | Sí | - |
dc.identifier.funder | http://dx.doi.org/10.13039/501100004794 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100003329 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100001659 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100004837 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.openairetype | artículo | - |
Aparece en las colecciones: | (IAA) Artículos (IFT) Artículos |
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IAA_2016_MNRASstw1483.pdf | 1,96 MB | Adobe PDF | Visualizar/Abrir |
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