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&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 recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2016 |
| País: | España |
| Institución: | Universidad de Barcelona |
| Repositorio: | Dipòsit Digital de la UB |
| OAI Identifier: | oai:diposit.ub.edu:2445/119250 |
| Acceso en línea: | https://hdl.handle.net/2445/119250 |
| Access Level: | acceso abierto |
| Palabra clave: | Cúmuls de galàxies Univers Clusters of galaxies Universe |
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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, Sergio A.Chuang, Chia-HsunZhao, ChengPrada, FranciscoGil Marín, HéctorGuo, HongYepes, GustavoKlypin, AnatolyScoccola, Claudia G.Tinker, Jeremy L.McBride, Cameron K.Reid, Beth A.Sánchez, Ariel G.Salazar-Albornoz, SalvadorNiklas Grieb, JanVargas Magaña, MarianaCuesta, Antonio J.Neyrinck, MarkBeutler, FlorianComparat, JohanPercival, Will J.Ross, Ashley J.Cúmuls de galàxiesUniversClusters of galaxiesUniverseWe reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11&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-1 Gpc]3 (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&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 1σ, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11&DR12 galaxy samples.Royal Astronomical Society2016info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/119250Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésReproducció del document publicat a: https://doi.org/10.1093/mnras/stv2826Monthly Notices of the Royal Astronomical Society, 2016, vol. 456, num. 4, p. 4156-4173https://doi.org/10.1093/mnras/stv2826info:eu-repo/grantAgreement/EC/FP7/240117(c) Kitaura, F.-S. et al., 2016info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/1192502026-05-27T06:46:51Z |
| 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 Cúmuls de galàxies Univers Clusters of galaxies 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 A. Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia G. Tinker, Jeremy L. McBride, Cameron K. Reid, Beth A. Sánchez, Ariel G. Salazar-Albornoz, Salvador Niklas Grieb, Jan Vargas Magaña, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley J. |
| author |
Kitaura, Francisco-Shu |
| author_facet |
Kitaura, Francisco-Shu Rodríguez Torres, Sergio A. Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia G. Tinker, Jeremy L. McBride, Cameron K. Reid, Beth A. Sánchez, Ariel G. Salazar-Albornoz, Salvador Niklas Grieb, Jan Vargas Magaña, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley J. |
| author_role |
author |
| author2 |
Rodríguez Torres, Sergio A. Chuang, Chia-Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia G. Tinker, Jeremy L. McBride, Cameron K. Reid, Beth A. Sánchez, Ariel G. Salazar-Albornoz, Salvador Niklas Grieb, Jan Vargas Magaña, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley J. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Cúmuls de galàxies Univers Clusters of galaxies Universe |
| topic |
Cúmuls de galàxies Univers Clusters of galaxies Universe |
| description |
We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11&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-1 Gpc]3 (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&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 1σ, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11&DR12 galaxy samples. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/2445/119250 |
| url |
https://hdl.handle.net/2445/119250 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
Reproducció del document publicat a: https://doi.org/10.1093/mnras/stv2826 Monthly Notices of the Royal Astronomical Society, 2016, vol. 456, num. 4, p. 4156-4173 https://doi.org/10.1093/mnras/stv2826 info:eu-repo/grantAgreement/EC/FP7/240117 |
| dc.rights.none.fl_str_mv |
(c) Kitaura, F.-S. et al., 2016 info:eu-repo/semantics/openAccess |
| rights_invalid_str_mv |
(c) Kitaura, F.-S. et al., 2016 |
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openAccess |
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application/pdf |
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Royal Astronomical Society |
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Royal Astronomical Society |
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Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB)) reponame:Dipòsit Digital de la UB instname:Universidad de Barcelona |
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Universidad de Barcelona |
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Dipòsit Digital de la UB |
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Dipòsit Digital de la UB |
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