The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample

We present 2000 mock galaxy catalogues for the analysis of baryon acoustic oscillations (BAOs) in the Emission Line Galaxy (ELG) sample of the extended Baryon Oscillation Spectroscopic Survey Data Release 16 (eBOSS DR16). Each mock catalogue has a number density of 6.7 x 10(-4)h(3)Mpc(-3), covering...

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Autores: Lin, Sicheng, Tinker, Jeremy L., Klypin, Anatoly, Prada, Francisco, Blanton, Michael R., Comparat, Johan, Dawson, Kyle, de Mattia, Arnaud, du Mas des Bourboux, Hélion, Percival, Will J., Raichoor, Anand, Rossi, Graziano, Smith, Alex, Zhao, Cheng
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/224431
Acceso en línea:http://hdl.handle.net/10261/224431
Access Level:acceso abierto
Palabra clave:Galaxies: haloes
Large-scale structure of the universe
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oai_identifier_str oai:digital.csic.es:10261/224431
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network_name_str España
repository_id_str
dc.title.none.fl_str_mv The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
title The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
spellingShingle The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
Lin, Sicheng
Galaxies: haloes
Large-scale structure of the universe
title_short The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
title_full The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
title_fullStr The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
title_full_unstemmed The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
title_sort The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample
dc.creator.none.fl_str_mv Lin, Sicheng
Tinker, Jeremy L.
Klypin, Anatoly
Prada, Francisco
Blanton, Michael R.
Comparat, Johan
Dawson, Kyle
de Mattia, Arnaud
du Mas des Bourboux, Hélion
Percival, Will J.
Raichoor, Anand
Rossi, Graziano
Smith, Alex
Zhao, Cheng
author Lin, Sicheng
author_facet Lin, Sicheng
Tinker, Jeremy L.
Klypin, Anatoly
Prada, Francisco
Blanton, Michael R.
Comparat, Johan
Dawson, Kyle
de Mattia, Arnaud
du Mas des Bourboux, Hélion
Percival, Will J.
Raichoor, Anand
Rossi, Graziano
Smith, Alex
Zhao, Cheng
author_role author
author2 Tinker, Jeremy L.
Klypin, Anatoly
Prada, Francisco
Blanton, Michael R.
Comparat, Johan
Dawson, Kyle
de Mattia, Arnaud
du Mas des Bourboux, Hélion
Percival, Will J.
Raichoor, Anand
Rossi, Graziano
Smith, Alex
Zhao, Cheng
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv National Science Foundation (US)
Ministerio de Ciencia, Innovación y Universidades (España)
European Commission
National Research Foundation of Korea
Sejong University
Alfred P. Sloan Foundation
Department of Energy (US)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: haloes
Large-scale structure of the universe
topic Galaxies: haloes
Large-scale structure of the universe
description We present 2000 mock galaxy catalogues for the analysis of baryon acoustic oscillations (BAOs) in the Emission Line Galaxy (ELG) sample of the extended Baryon Oscillation Spectroscopic Survey Data Release 16 (eBOSS DR16). Each mock catalogue has a number density of 6.7 x 10(-4)h(3)Mpc(-3), covering a redshift range from 0.6 to 1.1. The mocks are calibrated to small-scale eBOSS ELG clustering measurements at scales of less than or similar to 30 h(-1) Mpc. The mock catalogues are generated using a combination of GaLAxy Mocks (GLAM) simulations and the quick particle-mesh (QPM) method. GLAM simulations are used to generate the density field, which is then assigned dark matter haloes using the QPM method. Haloes are populated with galaxies using a halo occupation distribution. The resulting mocks match the survey geometry and selection function of the data, and have slightly higher number density that allows room for systematic analysis. The large-scale clustering of mocks at the BAO scale is consistent with data and we present the correlation matrix of the mocks. © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
publishDate 2020
dc.date.none.fl_str_mv 2020
2020
2020
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/224431
url http://hdl.handle.net/10261/224431
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/GC2018-101931-B-100
http://dx.doi.org/10.1093/mnras/staa2571
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869423328109789184
spelling The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sampleLin, SichengTinker, Jeremy L.Klypin, AnatolyPrada, FranciscoBlanton, Michael R.Comparat, JohanDawson, Kylede Mattia, Arnauddu Mas des Bourboux, HélionPercival, Will J.Raichoor, AnandRossi, GrazianoSmith, AlexZhao, ChengGalaxies: haloesLarge-scale structure of the universeWe present 2000 mock galaxy catalogues for the analysis of baryon acoustic oscillations (BAOs) in the Emission Line Galaxy (ELG) sample of the extended Baryon Oscillation Spectroscopic Survey Data Release 16 (eBOSS DR16). Each mock catalogue has a number density of 6.7 x 10(-4)h(3)Mpc(-3), covering a redshift range from 0.6 to 1.1. The mocks are calibrated to small-scale eBOSS ELG clustering measurements at scales of less than or similar to 30 h(-1) Mpc. The mock catalogues are generated using a combination of GaLAxy Mocks (GLAM) simulations and the quick particle-mesh (QPM) method. GLAM simulations are used to generate the density field, which is then assigned dark matter haloes using the QPM method. Haloes are populated with galaxies using a halo occupation distribution. The resulting mocks match the survey geometry and selection function of the data, and have slightly higher number density that allows room for systematic analysis. The large-scale clustering of mocks at the BAO scale is consistent with data and we present the correlation matrix of the mocks. © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical SocietySL is grateful to the support from CCPP, New York University. JLT and MRB are supported by NSF Award 1615997. FP and AK acknowledge support from the Spanish Ministry of Science and Innovation (MICINU) grant GC2018-101931-B-100. GR acknowledges support from the National Research Foundation of Korea (NRF) through grants nos. 2017R1E1A1A01077508 and 2020R1A2C1005655 funded by the Korean Ministry of Education, Science and Technology (MoEST), and from the faculty research fund of Sejong University. The GLAM simulations used in this paper were done on MareNostrum-4 at the Barcelona Supercomputer Center in Spain. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSSIV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org. SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrof ' isica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.Peer reviewedOxford University PressNational Science Foundation (US)Ministerio de Ciencia, Innovación y Universidades (España)European CommissionNational Research Foundation of KoreaSejong UniversityAlfred P. Sloan FoundationDepartment of Energy (US)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202020202020info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/224431reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/GC2018-101931-B-100http://dx.doi.org/10.1093/mnras/staa2571Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2244312026-05-22T06:33:51Z
score 15,811543

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