The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release
We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generat...
| Autores: | , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de documento: | artigo |
| Estado: | Versão publicada |
| Data de publicação: | 2016 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositório: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/376304 |
| Acesso em linha: | http://hdl.handle.net/10261/376304 |
| Access Level: | Acceso aberto |
| Palavra-chave: | Methods: numerical Galaxies: haloes Galaxies: statistics Large-scale structure of Universe |
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oai:digital.csic.es:10261/376304 |
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España |
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| dc.title.none.fl_str_mv |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| spellingShingle |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release Kitaura, Francisco-Shu Methods: numerical Galaxies: haloes Galaxies: statistics Large-scale structure of Universe |
| title_short |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_full |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_fullStr |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_full_unstemmed |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_sort |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| dc.creator.none.fl_str_mv |
Kitaura, Francisco-Shu Rodríguez-Torres, Sergio Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil-Marín, Héctor Guo, Hong ; Yepes, Gustavo Klypin, Anatoly Scóccola, Claudia G. Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar-Albornoz, Salvador Grieb, Jan Niklas Vargas-Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author |
Kitaura, Francisco-Shu |
| author_facet |
Kitaura, Francisco-Shu Rodríguez-Torres, Sergio Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil-Marín, Héctor Guo, Hong ; Yepes, Gustavo Klypin, Anatoly Scóccola, Claudia G. Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar-Albornoz, Salvador Grieb, Jan Niklas Vargas-Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author_role |
author |
| author2 |
Rodríguez-Torres, Sergio Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil-Marín, Héctor Guo, Hong ; Yepes, Gustavo Klypin, Anatoly Scóccola, Claudia G. Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar-Albornoz, Salvador Grieb, Jan Niklas Vargas-Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Ministerio de Ciencia e Innovación (España) Science and Technology Facilities Council (UK) Ministerio de Economía y Competitividad (España) German Research Foundation European Research Council European Commission National Energy Research Scientific Computing Center (US) Department of Energy (US) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Methods: numerical Galaxies: haloes Galaxies: statistics Large-scale structure of Universe |
| topic |
Methods: numerical Galaxies: haloes Galaxies: statistics Large-scale structure of Universe |
| description |
We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h Gpc] (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples. © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016 2025 2025 2025 |
| 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/10261/376304 |
| url |
http://hdl.handle.net/10261/376304 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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Oxford University Press |
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Oxford University Press |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data ReleaseKitaura, Francisco-ShuRodríguez-Torres, SergioChuang, Chia-HsunZhao, ChengPrada, FranciscoGil-Marín, HéctorGuo, Hong ; Yepes, GustavoKlypin, AnatolyScóccola, Claudia G.Tinker, JeremyMcBride, CameronReid, BethSánchez, Ariel G.Salazar-Albornoz, SalvadorGrieb, Jan NiklasVargas-Magana, MarianaCuesta, Antonio J.Neyrinck, MarkBeutler, FlorianComparat, JohanPercival, Will J.Ross, AshleyMethods: numericalGalaxies: haloesGalaxies: statisticsLarge-scale structure of UniverseWe reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h Gpc] (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples. © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.FSK, SRT, CC, CZ, FP, AK, and CGS acknowledge support from the Spanish MICINNs Consolider-Ingenio 2010 Programme under grant MultiDark CSD2009-00064, MINECO Centro de Excelencia Severo Ochoa Programme under grant SEV- 2012-0249, and grant AYA2014-60641-C2-1-P. FSK and CZ also want to thank the Instituto de Física Teórica UAM/CSIC for the hospitality and support during several visits, where part of this work was completed. FP wishes to thank the Lawrence Berkeley National Laboratory for the hospitality during the development of this work; he also acknowledges the Spanish MEC ‘Salvador de Madariaga’ programme, Ref. PRX14/00444. HGM is grateful for support from the UK Science and Technology Facilities Council through the grant ST/I001204/1. HG acknowledges the suppWith funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (SEV-2012-0249).Peer reviewedOxford University PressMinisterio de Ciencia e Innovación (España)Science and Technology Facilities Council (UK)Ministerio de Economía y Competitividad (España)German Research FoundationEuropean Research CouncilEuropean CommissionNational Energy Research Scientific Computing Center (US)Department of Energy (US)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2025202520162025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/376304reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO//SEV-2012-0249info:eu-repo/grantAgreement/MINECO//AYA2014-60641-C2-1-Pinfo:eu-repo/grantAgreement/MINECO//AYA2012-31101info:eu-repo/grantAgreement/EC/FP7/240117info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/MDM-2014-0369http://dx.doi.org/10.1093/mnras/stv2826Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3763042026-05-22T06:33:51Z |
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15,811543 |