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Title: The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights

Abstract

We develop a new method, which is based on the optimal redshift weighting scheme, to extract the maximal tomographic information of baryonic acoustic oscillations (BAO) and redshift space distortions (RSD) from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 14 quasar (DR14Q) survey. We validate our method using the Extended Zel’dovich mocks, and apply our pipeline to the eBOSS DR14Q sample in the redshift range of 0.8 < z < 2.2. We report a joint measurement of fσ8 and two-dimensional BAO parameters DA and H at four effective redshifts of zeff = 0.98, 1.23, 1.52, and 1.94, and provide the full data covariance matrix. Using our measurement combined with BOSS DR12, Main Galaxy Sample (MGS), and 6 degree Field Galaxy Survey (6dFGS) BAO measurements, we find that the existence of dark energy is supported by observations at a 7.4σ significance level. Combining our measurement with BOSS DR12 and Planck observations, we constrain the gravitational growth index to be γ = 0.580 ± 0.082, which is fully consistent with the prediction of general relativity. This paper is part of a set that analyses the eBOSS DR14 quasar sample.

Authors:
ORCiD logo [1];  [2];  [3];  [4];  [5];  [6];  [7];  [5];  [5];  [8]; ORCiD logo [9];  [10];  [11];  [12];  [13];  [6];  [14];  [14]; ORCiD logo [15];  [16] more »;  [17]; ORCiD logo [17];  [17];  [18];  [19];  [20]; ORCiD logo [21];  [22]; ORCiD logo [23];  [24]; ORCiD logo [25] « less
+ Show Author Affiliations
  1. Univ. of Portsmouth (United Kingdom); Chinese Academy of Sciences (CAS), Beijing (China); Univ. of Chinese Academy of Sciences, Beijing (China)
  2. Chinese Academy of Sciences (CAS), Beijing (China)
  3. Max Planck Society, Garching (Germany). Max Planck Inst. for Astrophysik
  4. Sorbonne Univ., Paris (France); Univ. Pierre et Marie Curie, Paris (France)
  5. Univ. of Portsmouth (United Kingdom)
  6. Chinese Academy of Sciences (CAS), Beijing (China); Univ. of Chinese Academy of Sciences, Beijing (China)
  7. Leibniz Inst. for Astrophysics Potsdam (AIP) (Germany); Stanford Univ., CA (United States)
  8. Yale Univ., New Haven, CT (United States)
  9. Univ. of Portsmouth (United Kingdom); The Ohio State Univ., Columbus, OH (United States)
  10. Univ. of St. Andrews, Scotland (United Kingdom)
  11. Aix-Marseille Univ., and CNRS/IN2P3, Marseille (France)
  12. Univ. of Wyoming, Laramie, WY (United States)
  13. New York Univ. (NYU), NY (United States)
  14. Univ. Paris-Saclay, Gif-sur-Yvette (France)
  15. Univ. of Portsmouth (United Kingdom); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  16. Leibniz Inst. for Astrophysics Potsdam (AIP) (Germany); Humboldt Univ. of Berlin (Germany)
  17. Univ. of Utah, Salt Lake City, UT (United States)
  18. Ludwig Maximilian Univ., Munich (Germany); Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
  19. Univ. Nacional Autonoma de Mexico (UNAM), Mexico City (Mexico)
  20. Sejong Univ., Seoul (Korea, Republic of)
  21. Univ. of Edinburgh, Scotland (United Kingdom). The Royal Observatory
  22. Max Planck Inst. fur Extraterrestrische Physik, Garching (Germany)
  23. Korea Astronmy and SPace Science Inst., Daejeon (Korea, Republic of); Univ. of Science and Technology, Daejon (Korea, Republic of)
  24. Pennsylvania State Univ., University Park, PA (United States)
  25. Chinese Academy of Sciences (CAS), Beijing (China); Tsinghua Univ., Beijing (China)
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Univ. of California, Oakland, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1543974
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 482; Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics

Citation Formats

Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Gil-Marín, Héctor, Percival, Will J., Wang, Dandan, Chuang, Chia-Hsun, Ruggeri, Rossana, Mueller, Eva-Maria, Zhu, Fangzhou, Ross, Ashley J., Tojeiro, Rita, Pâris, Isabelle, Myers, Adam D., Tinker, Jeremy L., Li, Jian, Burtin, Etienne, Zarrouk, Pauline, Beutler, Florian, Baumgarten, Falk, Bautista, Julian E., Brownstein, Joel R., Dawson, Kyle S., Hou, Jiamin, de la Macorra, Axel, Rossi, Graziano, Peacock, John A., Sánchez, Ariel G., Shafieloo, Arman, Schneider, Donald P., and Zhao, Cheng. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights. United States: N. p., 2018. Web. doi:10.1093/mnras/sty2845.
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Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Gil-Marín, Héctor, Percival, Will J., Wang, Dandan, Chuang, Chia-Hsun, Ruggeri, Rossana, Mueller, Eva-Maria, Zhu, Fangzhou, Ross, Ashley J., Tojeiro, Rita, Pâris, Isabelle, Myers, Adam D., Tinker, Jeremy L., Li, Jian, Burtin, Etienne, Zarrouk, Pauline, Beutler, Florian, Baumgarten, Falk, Bautista, Julian E., Brownstein, Joel R., Dawson, Kyle S., Hou, Jiamin, de la Macorra, Axel, Rossi, Graziano, Peacock, John A., Sánchez, Ariel G., Shafieloo, Arman, Schneider, Donald P., & Zhao, Cheng. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights. United States. doi:10.1093/mnras/sty2845.
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Zhao, Gong-Bo, Wang, Yuting, Saito, Shun, Gil-Marín, Héctor, Percival, Will J., Wang, Dandan, Chuang, Chia-Hsun, Ruggeri, Rossana, Mueller, Eva-Maria, Zhu, Fangzhou, Ross, Ashley J., Tojeiro, Rita, Pâris, Isabelle, Myers, Adam D., Tinker, Jeremy L., Li, Jian, Burtin, Etienne, Zarrouk, Pauline, Beutler, Florian, Baumgarten, Falk, Bautista, Julian E., Brownstein, Joel R., Dawson, Kyle S., Hou, Jiamin, de la Macorra, Axel, Rossi, Graziano, Peacock, John A., Sánchez, Ariel G., Shafieloo, Arman, Schneider, Donald P., and Zhao, Cheng. Fri . "The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights". United States. doi:10.1093/mnras/sty2845. https://www.osti.gov/servlets/purl/1543974.
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@article{osti_1543974,
title = {The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights},
author = {Zhao, Gong-Bo and Wang, Yuting and Saito, Shun and Gil-Marín, Héctor and Percival, Will J. and Wang, Dandan and Chuang, Chia-Hsun and Ruggeri, Rossana and Mueller, Eva-Maria and Zhu, Fangzhou and Ross, Ashley J. and Tojeiro, Rita and Pâris, Isabelle and Myers, Adam D. and Tinker, Jeremy L. and Li, Jian and Burtin, Etienne and Zarrouk, Pauline and Beutler, Florian and Baumgarten, Falk and Bautista, Julian E. and Brownstein, Joel R. and Dawson, Kyle S. and Hou, Jiamin and de la Macorra, Axel and Rossi, Graziano and Peacock, John A. and Sánchez, Ariel G. and Shafieloo, Arman and Schneider, Donald P. and Zhao, Cheng},
abstractNote = {We develop a new method, which is based on the optimal redshift weighting scheme, to extract the maximal tomographic information of baryonic acoustic oscillations (BAO) and redshift space distortions (RSD) from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 14 quasar (DR14Q) survey. We validate our method using the Extended Zel’dovich mocks, and apply our pipeline to the eBOSS DR14Q sample in the redshift range of 0.8 < z < 2.2. We report a joint measurement of fσ8 and two-dimensional BAO parameters DA and H at four effective redshifts of zeff = 0.98, 1.23, 1.52, and 1.94, and provide the full data covariance matrix. Using our measurement combined with BOSS DR12, Main Galaxy Sample (MGS), and 6 degree Field Galaxy Survey (6dFGS) BAO measurements, we find that the existence of dark energy is supported by observations at a 7.4σ significance level. Combining our measurement with BOSS DR12 and Planck observations, we constrain the gravitational growth index to be γ = 0.580 ± 0.082, which is fully consistent with the prediction of general relativity. This paper is part of a set that analyses the eBOSS DR14 quasar sample.},
doi = {10.1093/mnras/sty2845},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 482,
place = {United States},
year = {2018},
month = {10}
}
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DOI:  10.1093/mnras/sty2845
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Figures / Tables:

Figure 1 Figure 1: The observed volume number density (binned with $∆z$ = 0.05) of the quasars in unit of h3 Mpc−3 (multiplied by 105) as a function of redshifts in the NGC (upper black) and SGC (lower blue). The grey shaded region (0.8 < $z$ < 2.2) shows the redshift rangemore » in which data are selected for this analysis.« less
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    • de Sainte Agathe, Victoria; Balland, Christophe; du Mas des Bourboux, Hélion
    • Astronomy & Astrophysics, Vol. 629
    • DOI: 10.1051/0004-6361/201935638

    Nonparametric Dark Energy Reconstruction Using the Tomographic Alcock–Paczynski Test
    journal, June 2019

    Growth of matter perturbations in the bi-Galileons field model
    journal, December 2019

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