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Title: The clustering of theSDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the anisotropic baryon acoustic oscillations with redshift weights

Abstract

We present an anisotropic analysis of baryon acoustic oscillation (BAO) signal from the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 14 quasar sample. The sample consists of 147 000 quasars distributed over a redshift range of 0.8 < z < 2.2. We apply the redshift weights technique to the clustering of quasars in this sample and achieve a 4.6 per cent measurement of the angular distance measurement DM at z = 2.2 and Hubble parameter H at z = 0.8. We parametrize the distance-redshift relation, relative to a fiducial model, as a Taylor series. The coefficients of this expansion are used to reconstruct the distance-redshift relation and obtain distance and Hubble parameter measurements at all redshifts within the redshift range of the sample. Reporting the result at two characteristic redshifts, we determine DM(z = 1) = 3405 ± 305 (rd/rd, fid) Mpc, H(z=1) = 120.7± 7.3 (r_d,fid / r_d) km s^{-1} Mpc^{-1} and DM(z = 2) = 5325 ± 249 (rd/rd, fid) Mpc, H(z=2) = 189.9± 32.9 (r_d,fid / r_d) km s^{-1} Mpc^{-1}. These measurements are highly correlated. We assess the outlook of BAO analysis from the final quasar sample by testing the method onmore » a set of mocks that mimic the noise level in the final sample. We demonstrate on these mocks that redshift weighting shrinks the measurement error by over 25 per cent on average. We conclude redshift weighting can bring us closer to the cosmological goal of the final quasar sample.« less

Authors:
 [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3];  [4];  [4];  [5];  [6];  [4];  [7];  [8];  [9]; ORCiD logo [10];  [11]; ORCiD logo [9];  [9];  [12];  [13];  [14]; ORCiD logo [15] more »;  [5] « less
  1. Department of Physics, Yale University, New Haven, CT 06511, USA
  2. Center for Cosmology and Astroparticle Physics, Department of Physics, The Ohio State University, OH 43210, USA
  3. Department of Physics and Astronomy, U.C. Berkeley, Berkeley, CA 94720, USA
  4. Institute of Cosmology, Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth, PO1 3FX, UK
  5. Institute of Cosmology, Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth, PO1 3FX, UK; National Astronomy Observatories, Chinese Academy of Science, Beijing 100012, P.R. China
  6. National Astronomy Observatories, Chinese Academy of Science, Beijing 100012, P.R. China
  7. IRFU, CFA, Université Paris-Scalay, F-91191 Gif-sur-Yvette, France
  8. Sorbonne Universités, Institut Lagrange de Paris (ILP), 98 bis Boulevard Arago, 75014 Paris, France; Laboratoire de Physique Nucléaire et de Hautes Energies, Université Pierre et Marie Curie, 4 Place Jussieu, 75005 Paris, France
  9. Department of Physics and Astronomy, University of Utah, 115 S. 1400 E., Salt Lake City, UT 84112, USA
  10. Institute of Cosmology, Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth, PO1 3FX, UK; Lawrence Berkeley National Lab, 1 Cyclotron Rd, Berkeley CA 94720, USA
  11. Apache Point Observatory, PO Box 59, Sunspot, NM 88349, USA
  12. Instituto de Física, Universidad Nacional Autónoma de México, Apdo.Postal 20-364, 01000 México D.F., México
  13. Department of Physics and Astronomy, Sejong University, Seoul 143-747, Korea
  14. Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
  15. School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK
Publication Date:
Research Org.:
Univ. of California, Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25); National Science Foundation (NSF)
OSTI Identifier:
1594729
Alternate Identifier(s):
OSTI ID: 1593672
Grant/Contract Number:  
SC0017860; AC02-05CH11231; PHYS-1066293
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 480; Journal Issue: 1; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dark energy; distance scale; cosmology: observations

Citation Formats

Zhu, Fangzhou, Padmanabhan, Nikhil, Ross, Ashley J., White, Martin, Percival, Will J., Ruggeri, Rossana, Zhao, Gong-bo, Wang, Dandan, Mueller, Eva-Maria, Burtin, Etienne, Gil-Marín, Héctor, Bautista, Julian, Beutler, Florian, Brinkmann, Jonathan, Brownstein, Joel R., Dawson, Kyle, de la Macorra, Axel, Rossi, Graziano, Schneider, Donald P., Tojeiro, Rita, and Wang, Yuting. The clustering of theSDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the anisotropic baryon acoustic oscillations with redshift weights. United States: N. p., 2018. Web. doi:10.1093/mnras/sty1955.
Zhu, Fangzhou, Padmanabhan, Nikhil, Ross, Ashley J., White, Martin, Percival, Will J., Ruggeri, Rossana, Zhao, Gong-bo, Wang, Dandan, Mueller, Eva-Maria, Burtin, Etienne, Gil-Marín, Héctor, Bautista, Julian, Beutler, Florian, Brinkmann, Jonathan, Brownstein, Joel R., Dawson, Kyle, de la Macorra, Axel, Rossi, Graziano, Schneider, Donald P., Tojeiro, Rita, & Wang, Yuting. The clustering of theSDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the anisotropic baryon acoustic oscillations with redshift weights. United States. doi:10.1093/mnras/sty1955.
Zhu, Fangzhou, Padmanabhan, Nikhil, Ross, Ashley J., White, Martin, Percival, Will J., Ruggeri, Rossana, Zhao, Gong-bo, Wang, Dandan, Mueller, Eva-Maria, Burtin, Etienne, Gil-Marín, Héctor, Bautista, Julian, Beutler, Florian, Brinkmann, Jonathan, Brownstein, Joel R., Dawson, Kyle, de la Macorra, Axel, Rossi, Graziano, Schneider, Donald P., Tojeiro, Rita, and Wang, Yuting. Mon . "The clustering of theSDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the anisotropic baryon acoustic oscillations with redshift weights". United States. doi:10.1093/mnras/sty1955. https://www.osti.gov/servlets/purl/1594729.
@article{osti_1594729,
title = {The clustering of theSDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the anisotropic baryon acoustic oscillations with redshift weights},
author = {Zhu, Fangzhou and Padmanabhan, Nikhil and Ross, Ashley J. and White, Martin and Percival, Will J. and Ruggeri, Rossana and Zhao, Gong-bo and Wang, Dandan and Mueller, Eva-Maria and Burtin, Etienne and Gil-Marín, Héctor and Bautista, Julian and Beutler, Florian and Brinkmann, Jonathan and Brownstein, Joel R. and Dawson, Kyle and de la Macorra, Axel and Rossi, Graziano and Schneider, Donald P. and Tojeiro, Rita and Wang, Yuting},
abstractNote = {We present an anisotropic analysis of baryon acoustic oscillation (BAO) signal from the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 14 quasar sample. The sample consists of 147 000 quasars distributed over a redshift range of 0.8 < z < 2.2. We apply the redshift weights technique to the clustering of quasars in this sample and achieve a 4.6 per cent measurement of the angular distance measurement DM at z = 2.2 and Hubble parameter H at z = 0.8. We parametrize the distance-redshift relation, relative to a fiducial model, as a Taylor series. The coefficients of this expansion are used to reconstruct the distance-redshift relation and obtain distance and Hubble parameter measurements at all redshifts within the redshift range of the sample. Reporting the result at two characteristic redshifts, we determine DM(z = 1) = 3405 ± 305 (rd/rd, fid) Mpc, H(z=1) = 120.7± 7.3 (r_d,fid / r_d) km s^{-1} Mpc^{-1} and DM(z = 2) = 5325 ± 249 (rd/rd, fid) Mpc, H(z=2) = 189.9± 32.9 (r_d,fid / r_d) km s^{-1} Mpc^{-1}. These measurements are highly correlated. We assess the outlook of BAO analysis from the final quasar sample by testing the method on a set of mocks that mimic the noise level in the final sample. We demonstrate on these mocks that redshift weighting shrinks the measurement error by over 25 per cent on average. We conclude redshift weighting can bring us closer to the cosmological goal of the final quasar sample.},
doi = {10.1093/mnras/sty1955},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 480,
place = {United States},
year = {2018},
month = {7}
}

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