Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters
Abstract
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 Vceil 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.
- Authors:
-
[1];
[2];
[1];
[6];
[7];
- 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)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Research Foundation of Korea (NRF); Alfred P. Sloan Foundation; Swiss National Science Foundation (SNSF)
- OSTI Identifier:
- 1906705
- Grant/Contract Number:
- AC02-05CH11231; 2020R1A2C1005655; SNF 200020_175751
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 516; Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; numerical method; observational method; halo; large-scale structure of the universe
Citation Formats
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, and Rossi, Graziano. Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters. United States: N. p., 2022.
Web. doi:10.1093/mnras/stac2176.
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. Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters. United States. https://doi.org/10.1093/mnras/stac2176
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, and Rossi, Graziano. Wed .
"Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters". United States. https://doi.org/10.1093/mnras/stac2176. https://www.osti.gov/servlets/purl/1906705.
@article{osti_1906705,
title = {Model BOSS and eBOSS luminous red galaxies at 0.2< z<1.0 using SubHalo Abundance Matching with three parameters},
author = {Yu, Jiaxi and Zhao, Cheng and Chuang, Chia-Hsun and Bautista, Julian E. and Favole, Ginevra and Kneib, Jean-Paul and Mohammad, Faizan G. and Ross, Ashley J. and Raichoor, Anand and Tao, Charling and Dawson, Kyle and Rossi, Graziano},
abstractNote = {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 Vceil 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.},
doi = {10.1093/mnras/stac2176},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 516,
place = {United States},
year = {Wed Aug 03 00:00:00 EDT 2022},
month = {Wed Aug 03 00:00:00 EDT 2022}
}
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- Madau, Piero; Pozzetti, Lucia; Dickinson, Mark
- The Astrophysical Journal, Vol. 498, Issue 1
Bias and variance of angular correlation functions
journal, July 1993
- Landy, Stephen D.; Szalay, Alexander S.
- The Astrophysical Journal, Vol. 412
Clustering in real space and in redshift space
journal, July 1987
- Kaiser, Nick
- Monthly Notices of the Royal Astronomical Society, Vol. 227, Issue 1
Building a better understanding of the massive high-redshift BOSS CMASS galaxies as tools for cosmology
journal, July 2016
- Favole, Ginevra; McBride, Cameron K.; Eisenstein, Daniel J.
- Monthly Notices of the Royal Astronomical Society, Vol. 462, Issue 2
How do galaxies populate dark matter haloes?
journal, March 2010
- Guo, Qi; White, Simon; Li, Cheng
- Monthly Notices of the Royal Astronomical Society
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis
journal, September 2020
- Ross, Ashley J.; Bautista, Julian; Tojeiro, Rita
- Monthly Notices of the Royal Astronomical Society, Vol. 498, Issue 2
Modeling Galaxy‐Mass Correlations in Dissipationless Simulations
journal, October 2004
- Tasitsiomi, Argyro; Kravtsov, Andrey V.; Wechsler, Risa H.
- The Astrophysical Journal, Vol. 614, Issue 2
Clustering properties of g -selected galaxies at z ∼ 0.8
journal, June 2016
- Favole, Ginevra; Comparat, Johan; Prada, Francisco
- Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 4
The Radial Distribution of Galaxies in Λ Cold Dark Matter Clusters
journal, January 2005
- Nagai, Daisuke; Kravtsov, Andrey V.
- The Astrophysical Journal, Vol. 618, Issue 2