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  The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multitracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate

Zhao, G.-B., Wang, Y., Taruya, A., Zhang, W., Gil-Marín, H., de Mattia, A., et al. (2021). The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multitracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate. Monthly Notices of the Royal Astronomical Society, 504(1), 33-52. doi:10.1093/mnras/stab849.

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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey a multitracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate.pdf (Any fulltext), 4MB
 
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 Creators:
Zhao, Gong-Bo, Author
Wang, Yuting, Author
Taruya, Atsushi, Author
Zhang, Weibing, Author
Gil-Marín, Héctor, Author
de Mattia, Arnaud, Author
Ross, Ashley J, Author
Raichoor, Anand, Author
Zhao, Cheng, Author
Percival, Will J, Author
Alam, Shadab, Author
Bautista, Julian E, Author
Burtin, Etienne, Author
Chuang, Chia-Hsun, Author
Dawson, Kyle S, Author
Hou, Jiamin1, Author           
Kneib, Jean-Paul, Author
Koyama, Kazuya, Author
du Bourboux, Hélion Mas des, Author
Mueller, Eva-Maria, Author
Newman, Jeffrey A, AuthorPeacock, John A, AuthorRossi, Graziano, AuthorRuhlmann-Kleider, Vanina, AuthorSchneider, Donald P, AuthorShafieloo, Arman, Author more..
Affiliations:
1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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 Abstract: We perform a joint BAO and RSD analysis using the eBOSS DR16 LRG and ELG samples in the redshift range of z ∈ [0.6, 1.1], and detect an RSD signal from the cross-power spectrum at a ∼4σ confidence level, i.e., fσ8 = 0.317 ± 0.080 at zeff = 0.77. Based on the chained power spectrum, which is a new development in this work to mitigate the angular systematics, we measure the BAO distances and growth rate simultaneously at two effective redshifts, namely, DM/rd (z = 0.70) = 17.96 ± 0.51, DH/rd (z = 0.70) = 21.22 ± 1.20, fσ8 (z = 0.70) = 0.43 ± 0.05, and DM/rd (z = 0.845) = 18.90 ± 0.78, DH/rd (z = 0.845) = 20.91 ± 2.86, fσ8 (z = 0.845) = 0.30 ± 0.08. Combined with BAO measurements including those from the eBOSS DR16 QSO and Lyman-α sample, our measurement has raised the significance level of a non-zero ΩΛ to ∼11σ. The data product of this work is publicly available at https://github.com/icosmology/eBOSS_DR16_LRGxELG and https://www.sdss.org/science/final-bao-and-rsd-measurements/.

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Language(s): eng - English
 Dates: 2021-03-24
 Publication Status: Published online
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 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stab849
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 504 (1) Sequence Number: - Start / End Page: 33 - 52 Identifier: ISSN: 0035-8711
ISSN: 1365-8711