The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: growth rate of structure measurement from cosmic voids

Aubert, Marie; Cousinou, Marie-Claude; Escoffier, Stéphanie; Hawken, Adam J.; Nadathur, Seshadri; Alam, Shadab; Bautista, Julian; Burtin, Etienne; Chuang, Chia-Hsun; de la Macorra, Axel; de Mattia, Arnaud; Gil-Marín, Héctor; Hou, Jiamin; Jullo, Eric; Kneib, Jean-Paul; Neveux, Richard; Rossi, Graziano; Schneider, Donald; Smith, Alex; Tamone, Amélie; Vargas Magaña, Mariana; Zhao, Cheng

doi:10.1093/mnras/stac828

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: growth rate of structure measurement from cosmic voids

Journal Article · Sat Mar 26 00:00:00 EDT 2022 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stac828· OSTI ID:1864377

Aubert, Marie; Cousinou, Marie-Claude; Escoffier, Stéphanie; Hawken, Adam J.; ; Alam, Shadab; ; Burtin, Etienne; ; de la Macorra, Axel; de Mattia, Arnaud; ; Hou, Jiamin; Jullo, Eric; Kneib, Jean-Paul; Neveux, Richard; Rossi, Graziano; Schneider, Donald; Smith, Alex; Tamone, Amélie more »

ABSTRACT

We present a void clustering analysis in configuration-space using the completed Sloan Digital Sky Survey IV (SDSS-IV) extended Baryon Oscillation Spectroscopic Survey (eBOSS) DR16 samples. These samples consist of Luminous Red Galaxies (LRGs) combined with the high-redshift tail of the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) DR12 CMASS galaxies (called as LRG+CMASS sample), Emission Line Galaxies (ELGs), and quasars (QSOs). We build void catalogues from the three eBOSS DR16 samples using a ZOBOV-based algorithm, providing 2814 voids, 1801 voids, and 4347 voids in the LRG+CMASS, ELG, and QSO samples, respectively, spanning the redshift range 0.6 < z < 2.2. We measure the redshift space distortions around voids using the anisotropic void-galaxy cross-correlation function and we extract the distortion parameter β. We test the methodology on realistic simulations before applying it to the data, and we investigate all our systematic errors on these mocks. We find βLRG(z = 0.74) = 0.415 ± 0.087, βELG(z = 0.85) = 0.665 ± 0.125 and βQSO(z = 1.48) = 0.313 ± 0.134, for the LRG+CMASS, ELG, and QSO sample, respectively. The quoted errors include systematic and statistical contributions. In order to convert our measurements in terms of the growth rate fσ8, we use consensus values of linear bias from the eBOSS DR16 companion papers, resulting in the following constraints: fσ8(z = 0.74) = 0.50 ± 0.11, fσ8(z = 0.85) = 0.52 ± 0.10, and fσ8(z = 1.48) = 0.30 ± 0.13. Our measurements are consistent with other measurements from eBOSS DR16 using conventional clustering techniques.

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Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)

Sponsoring Organization:: European Research Council (ERC); French National Research Agency (ANR); Korean Ministry of Education, Science and Technology (MoEST); National Research Foundation of Korea (NRF); USDOE; USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities (SUF)

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1864377

Alternate ID(s):: OSTI ID: 1982701

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 513; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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The DESI Experiment Part II: Instrument Design Collaboration, Desi; Aghamousa, Amir; Aguilar, Jessica arXiv https://doi.org/10.48550/ARXIV.1611.00037	preprint	January 2016

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