Model BOSS and eBOSS luminous red galaxies at 0.2&lt; z&lt;1.0 using SubHalo Abundance Matching with three parameters

Yu, Jiaxi; Zhao, Cheng; Chuang, Chia-Hsun; Bautista, Julian E.; Favole, Ginevra; Kneib, Jean-Paul; Mohammad, Faizan G.; Ross, Ashley J.; Raichoor, Anand; Tao, Charling; Dawson, Kyle; Rossi, Graziano

doi:10.1093/mnras/stac2176

Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters

Journal Article · Wed Aug 03 00:00:00 EDT 2022 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stac2176· OSTI ID:1906705

Yu, Jiaxi ^[1]; ^[1]; ^[2]; Bautista, Julian E. ^[3]; ^[1]; Kneib, Jean-Paul ^[4]; Mohammad, Faizan G. ^[5]; ^[6]; ^[7]; Tao, Charling ^[3]; Dawson, Kyle ^[8]; Rossi, Graziano ^[9]

Ecole Polytechnique Federale Lausanne (EPFL) (Switzerland)
Univ. of Utah, Salt Lake City, UT (United States); Stanford Univ., CA (United States)
Aix-Marseille Univ., Marseille (France)
Ecole Polytechnique Federale Lausanne (EPFL) (Switzerland); Aix-Marseille Univ., Marseille (France)
Univ. of Waterloo, ON (Canada)
The Ohio State Univ., Columbus, OH (United States)
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Univ. of Utah, Salt Lake City, UT (United States)
Sejong Univ., Seoul (Korea, Republic of)

SubHalo Abundance Matching (SHAM) is an empirical method for constructing galaxy catalogues based on high-resolution N-body simulations. Here, we apply SHAM on the UNIT simulation to simulate SDSS BOSS/eBOSS luminous red galaxies (LRGs) within a wide redshift range of 0.2 < $$z$$ < 1.0. Besides the typical SHAM scatter parameter σ, we include $$v$$_smear and V_ceil to take into account the redshift uncertainty and the galaxy incompleteness, respectively. These two additional parameters are critical for reproducing the observed 2PCF multipoles on 5–25$$\, h^{-1}\, {\rm Mpc}$$. The redshift uncertainties obtained from the best-fitting $$v$$_smear agree with those measured from repeat observations for all SDSS LRGs except for the LOWZ sample. We explore several potential systematics but none of them can explain the discrepancy found in LOWZ. Our explanation is that the LOWZ galaxies might contain another type of galaxies that needs to be treated differently. The evolution of the measured σ and Vceil also reveals that the incompleteness of eBOSS galaxies decreases with the redshift. This is the consequence of the magnitude lower limit applied in eBOSS LRG target selection. Our SHAM also set upper limits for the intrinsic scatter of the galaxy–halo relation, given a complete galaxy sample: ^σint < 0.31 for LOWZ at 0.2 < $$z$$ < 0.33, ^σint < 0.36 for LOWZ at 0.33 < $$z$$ < 0.43, and ^σint < 0.46 for CMASS at 0.43 < $$z$$ < 0.51. The projected 2PCFs of our SHAM galaxies also agree with the observational ones on the 2PCF fitting range.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: Alfred P. Sloan Foundation; National Research Foundation of Korea (NRF); Swiss National Science Foundation; USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1906705

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 516; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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The Sdss-Iv Extended Baryon Oscillation Spectroscopic Survey: Luminous red Galaxy Target Selection Prakash, Abhishek; Licquia, Timothy C.; Newman, Jeffrey A. The Astrophysical Journal Supplement Series, Vol. 224, Issue 2 https://doi.org/10.3847/0067-0049/224/2/34	journal	June 2016
Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe Blanton, Michael R.; Bershady, Matthew A.; Abolfathi, Bela The Astronomical Journal, Vol. 154, Issue 1 https://doi.org/10.3847/1538-3881/aa7567	journal	June 2017
Overview of the DESI Legacy Imaging Surveys Dey, Arjun; Schlegel, David J.; Lang, Dustin The Astronomical Journal, Vol. 157, Issue 5 https://doi.org/10.3847/1538-3881/ab089d	journal	April 2019
The Mass–Concentration Relation and the Stellar-to-halo Mass Ratio in the CFHT Stripe 82 Survey Shan, HuanYuan; Kneib, Jean-Paul; Li, Ran The Astrophysical Journal, Vol. 840, Issue 2 https://doi.org/10.3847/1538-4357/aa6c68	journal	May 2017
The Clustering of Luminous Red Galaxies at z ∼ 0.7 from EBOSS and BOSS Data Zhai, Zhongxu; Tinker, Jeremy L.; Hahn, ChangHoon The Astrophysical Journal, Vol. 848, Issue 2 https://doi.org/10.3847/1538-4357/aa8eee	journal	October 2017
The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Ly α Forests du Mas des Bourboux, Hélion; Rich, James; Font-Ribera, Andreu The Astrophysical Journal, Vol. 901, Issue 2 https://doi.org/10.3847/1538-4357/abb085	journal	October 2020
The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra Ahumada, Romina; Prieto, Carlos Allende; Almeida, Andrés The Astrophysical Journal Supplement Series, Vol. 249, Issue 1 https://doi.org/10.3847/1538-4365/ab929e	journal	June 2020
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release Lyke, Brad W.; Higley, Alexandra N.; McLane, J. N. The Astrophysical Journal Supplement Series, Vol. 250, Issue 1 https://doi.org/10.3847/1538-4365/aba623	journal	August 2020

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