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Title: The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2

Abstract

We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space using the clustering of quasars. We consider a sample of 147,000 quasars from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) distributed over 2044 square degrees with redshifts $0.8 < z < 2.2$ and measure their spherically-averaged clustering in both configuration and Fourier space. Our observational dataset and the 1400 simulated realizations of the dataset allow us to detect a preference for BAO that is greater than 2.5$$\sigma$$. We determine the spherically averaged BAO distance to $z = 1.52$ to 4.4 per cent precision: $$D_V(z=1.52)=3855\pm170 \left(r_{\rm d}/r_{\rm d, fid}\right)\ $$Mpc. This is the first time the location of the BAO feature has been measured between redshifts 1 and 2. Our result is fully consistent with the prediction obtained by extrapolating the Planck flat $$\Lambda$$CDM best-fit cosmology. All of our results are consistent with basic large-scale structure (LSS) theory, confirming quasars to be a reliable tracer of LSS, and provide a starting point for numerous cosmological tests to be performed with eBOSS quasar samples. We combine our result with previous, independent, BAO distance measurements to construct an updated BAO distance-ladder. Using these BAO data alone and marginalizing over the length of the standard ruler, we find $$\Omega_{\Lambda} > 0$$ at 6.5$$\sigma$$ significance when testing a $$\Lambda$$CDM model with free curvature.

Authors:
 [1];  [2];  [3]; ORCiD logo [4];  [5];  [6];  [7];  [8];  [9];  [3];  [10];  [1];  [11];  [3];  [12];  [13];  [14];  [15];  [16];  [9] more »;  [17];  [18];  [19];  [3];  [20];  [21];  [22];  [14];  [14];  [23];  [4];  [3];  [24];  [14];  [9];  [25];  [21];  [4];  [26];  [27];  [28];  [29]; ORCiD logo [30];  [31];  [4];  [11];  [32];  [33];  [34];  [35];  [36];  [21];  [6]; ORCiD logo [37];  [12];  [3];  [38];  [39];  [40];  [14];  [40];  [38];  [41] « less
  1. Leibniz Inst. for Astrophysics (AIP), Potsdam (Germany)
  2. Leibniz Inst. for Astrophysics (AIP), Potsdam (Germany); Humboldt Univ. of Berlin (Germany). Inst. of Physics
  3. Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
  4. Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
  5. Apache Point Observatory and New Mexico State Univ., Sunspot, NM (United States); Moscow State Univ., Moscow (Russian Federation). Sternberg Astronomical Inst.
  6. New York Univ. (NYU), NY (United States). Center for Cosmology and Particle Physics
  7. Ecole Polytechnique Federale Lausanne (Switzlerland). Inst. of Physics
  8. Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy; National Optical Astronomy Observatory, Tucson, AZ (United States)
  9. Apache Point Observatory and New Mexico State Univ., Sunspot, NM (United States)
  10. Univ. of Paris-Saclay, Gif-sur-Yvette (France
  11. Max Planck Inst. for Extraterrestrial Physics, Munich (Germany)
  12. National Autonomous Univ. of Mexico (Mexico). Inst. of Physics
  13. Chinese Academy of Sciences (CAS), Beijing (China). National Astronomy Observatories
  14. Univ. of Paris-Saclay, Gif-sur-Yvette (France)
  15. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  16. Sorbonne Univ., Paris (France); Univ. Pierre et Marie Curie, Paris (France). Lab. of Nuclear Physics and High Energy
  17. Univ. Pierre et Marie Curie, Paris (France)
  18. Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
  19. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Carnegie Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics; Univ. of California, Berkeley, CA (United States). Berkeley Center for Cosmological Physics, Dept. of Physics
  20. Ecole Polytechnique Federale Lausanne (Switzlerland). Inst. of Physics; Russian Academy of Sciences (RAS), Moscow (Russian Federation). Inst. for Nuclear Research
  21. Institute of Astrophysics of the Canary Islands (IAC), La Laguna (Spain); Univ. of La Laguna (Spain)
  22. Ecole Polytechnique Federale Lausanne (Switzlerland). Inst. of Physics; Aix-Marseille Univ., Marseille (France)
  23. The Ohio State Univ., Columbus, OH (United States). Center for Cosmology and Astro-Particle Physics
  24. Univ. of Pittsburgh, PA (United States). Dept. of Physics and Astronomy, Pittsburgh Particle Physics, Astrophysics and Cosmology Center
  25. Aix-Marseille Univ., Marseille (France)
  26. Univ. of Paris (France). Inst. of Astrophysics
  27. Autonomous Univ. of Madrid (Spain). Inst. of Theoretical Physics; Campus of International Excellence, Madrid (Spain); Inst. of Astrophysics of Andalucia, Granada (Spain)
  28. Univ. of Pittsburgh, PA (United States). Dept. of Physics, Astronomy and the Pittsburgh Partice Physics, Astrophysics and Cosmology Center
  29. Autonomous Univ. of Madrid (Spain). Inst. of Theoretical Physics, Dept. of Theoretical Physics; Campus of International Excellence, Madrid (Spain)
  30. Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; The Ohio State Univ., Columbus, OH (United States). Center for Cosmology and Astro Particle Physics
  31. Sejong Univ., Seoul (Korea, Republic of). Dept. of Physics and Astronomy
  32. Carnegie Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics; Univ. of La Laguna (ULL) (Spain). Dept. of Astrophysics
  33. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  34. Pennsylvania State Univ., University Park, PA (United States). Dept. of Astronomy and Astrophysics, Inst. for Gravitation and the Cosmos
  35. The Ohio State Univ., Columbus, OH (United States). Dept. of Physics and Astronomy
  36. Brookhaven National Lab. (BNL), Upton, NY (United States)
  37. Univ. of St. Andrews, Scotland (United Kingdom). School of Physics and Astronomy
  38. Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation; Chinese Academy of Sciences (CAS), Beijing (China). National Astronomy Observatories
  39. Univ. of Paris-Saclay, Gif-sur-Yvette (France); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  40. Tsinghua Univ., Beijing (China). Tsinghua Center for Astrophysics, Dept. of Physics
  41. Yale Univ., New Haven, CT (United States). Dept. of Physics
Publication Date:
Research Org.:
The Ohio State Univ., Columbus, OH (United States); Brookhaven National Laboratory (BNL), Upton, NY (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1602479
Alternate Identifier(s):
OSTI ID: 1392224; OSTI ID: 1398497
Report Number(s):
BNL-114222-2017-JA
Journal ID: ISSN 0035-8711; TRN: US2104020
Grant/Contract Number:  
SC0011726; SC0012704; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 473; Journal Issue: 4; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; cosmology: large-scale structure of Universe

Citation Formats

Ata, Metin, Baumgarten, Falk, Bautista, Julian, Beutler, Florian, Bizyaev, Dmitry, Blanton, Michael R., Blazek, Jonathan A., Bolton, Adam S., Brinkmann, Jonathan, Brownstein, Joel R., Burtin, Etienne, Chuang, Chia-Hsun, Comparat, Johan, Dawson, Kyle S., de la Macorra, Axel, Du, Wei, du Mas des Bourboux, Hélion, Eisenstein, Daniel J., Gil-Marín, Héctor, Grabowski, Katie, Guy, Julien, Hand, Nick, Ho, Shirley, Hutchinson, Timothy A., Ivanov, Mikhail M., Kitaura, Francisco-Shu, Kneib, Jean-Paul, Laurent, Pierre, Le Goff, Jean-Marc, McEwen, Joseph E., Mueller, Eva-Maria, Myers, Adam D., Newman, Jeffrey A., Palanque-Delabrouille, Nathalie, Pan, Kaike, Pâris, Isabelle, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Prakash, Abhishek, Rodríguez-Torres, Sergio A., Ross, Ashley J., Rossi, Graziano, Ruggeri, Rossana, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Slosar, Anže, Streblyanska, Alina, Tinker, Jeremy L., Tojeiro, Rita, Vargas Magaña, Mariana, Vivek, M., Wang, Yuting, Yèche, Christophe, Yu, Liang, Zarrouk, Pauline, Zhao, Cheng, Zhao, Gong-Bo, and Zhu, Fangzhou. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2. United States: N. p., 2017. Web. doi:10.1093/mnras/stx2630.
Ata, Metin, Baumgarten, Falk, Bautista, Julian, Beutler, Florian, Bizyaev, Dmitry, Blanton, Michael R., Blazek, Jonathan A., Bolton, Adam S., Brinkmann, Jonathan, Brownstein, Joel R., Burtin, Etienne, Chuang, Chia-Hsun, Comparat, Johan, Dawson, Kyle S., de la Macorra, Axel, Du, Wei, du Mas des Bourboux, Hélion, Eisenstein, Daniel J., Gil-Marín, Héctor, Grabowski, Katie, Guy, Julien, Hand, Nick, Ho, Shirley, Hutchinson, Timothy A., Ivanov, Mikhail M., Kitaura, Francisco-Shu, Kneib, Jean-Paul, Laurent, Pierre, Le Goff, Jean-Marc, McEwen, Joseph E., Mueller, Eva-Maria, Myers, Adam D., Newman, Jeffrey A., Palanque-Delabrouille, Nathalie, Pan, Kaike, Pâris, Isabelle, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Prakash, Abhishek, Rodríguez-Torres, Sergio A., Ross, Ashley J., Rossi, Graziano, Ruggeri, Rossana, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Slosar, Anže, Streblyanska, Alina, Tinker, Jeremy L., Tojeiro, Rita, Vargas Magaña, Mariana, Vivek, M., Wang, Yuting, Yèche, Christophe, Yu, Liang, Zarrouk, Pauline, Zhao, Cheng, Zhao, Gong-Bo, & Zhu, Fangzhou. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2. United States. https://doi.org/10.1093/mnras/stx2630
Ata, Metin, Baumgarten, Falk, Bautista, Julian, Beutler, Florian, Bizyaev, Dmitry, Blanton, Michael R., Blazek, Jonathan A., Bolton, Adam S., Brinkmann, Jonathan, Brownstein, Joel R., Burtin, Etienne, Chuang, Chia-Hsun, Comparat, Johan, Dawson, Kyle S., de la Macorra, Axel, Du, Wei, du Mas des Bourboux, Hélion, Eisenstein, Daniel J., Gil-Marín, Héctor, Grabowski, Katie, Guy, Julien, Hand, Nick, Ho, Shirley, Hutchinson, Timothy A., Ivanov, Mikhail M., Kitaura, Francisco-Shu, Kneib, Jean-Paul, Laurent, Pierre, Le Goff, Jean-Marc, McEwen, Joseph E., Mueller, Eva-Maria, Myers, Adam D., Newman, Jeffrey A., Palanque-Delabrouille, Nathalie, Pan, Kaike, Pâris, Isabelle, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Prakash, Abhishek, Rodríguez-Torres, Sergio A., Ross, Ashley J., Rossi, Graziano, Ruggeri, Rossana, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Slosar, Anže, Streblyanska, Alina, Tinker, Jeremy L., Tojeiro, Rita, Vargas Magaña, Mariana, Vivek, M., Wang, Yuting, Yèche, Christophe, Yu, Liang, Zarrouk, Pauline, Zhao, Cheng, Zhao, Gong-Bo, and Zhu, Fangzhou. Tue . "The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2". United States. https://doi.org/10.1093/mnras/stx2630. https://www.osti.gov/servlets/purl/1602479.
@article{osti_1602479,
title = {The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: first measurement of baryon acoustic oscillations between redshift 0.8 and 2.2},
author = {Ata, Metin and Baumgarten, Falk and Bautista, Julian and Beutler, Florian and Bizyaev, Dmitry and Blanton, Michael R. and Blazek, Jonathan A. and Bolton, Adam S. and Brinkmann, Jonathan and Brownstein, Joel R. and Burtin, Etienne and Chuang, Chia-Hsun and Comparat, Johan and Dawson, Kyle S. and de la Macorra, Axel and Du, Wei and du Mas des Bourboux, Hélion and Eisenstein, Daniel J. and Gil-Marín, Héctor and Grabowski, Katie and Guy, Julien and Hand, Nick and Ho, Shirley and Hutchinson, Timothy A. and Ivanov, Mikhail M. and Kitaura, Francisco-Shu and Kneib, Jean-Paul and Laurent, Pierre and Le Goff, Jean-Marc and McEwen, Joseph E. and Mueller, Eva-Maria and Myers, Adam D. and Newman, Jeffrey A. and Palanque-Delabrouille, Nathalie and Pan, Kaike and Pâris, Isabelle and Pellejero-Ibanez, Marcos and Percival, Will J. and Petitjean, Patrick and Prada, Francisco and Prakash, Abhishek and Rodríguez-Torres, Sergio A. and Ross, Ashley J. and Rossi, Graziano and Ruggeri, Rossana and Sánchez, Ariel G. and Satpathy, Siddharth and Schlegel, David J. and Schneider, Donald P. and Seo, Hee-Jong and Slosar, Anže and Streblyanska, Alina and Tinker, Jeremy L. and Tojeiro, Rita and Vargas Magaña, Mariana and Vivek, M. and Wang, Yuting and Yèche, Christophe and Yu, Liang and Zarrouk, Pauline and Zhao, Cheng and Zhao, Gong-Bo and Zhu, Fangzhou},
abstractNote = {We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space using the clustering of quasars. We consider a sample of 147,000 quasars from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) distributed over 2044 square degrees with redshifts $0.8 < z < 2.2$ and measure their spherically-averaged clustering in both configuration and Fourier space. Our observational dataset and the 1400 simulated realizations of the dataset allow us to detect a preference for BAO that is greater than 2.5$\sigma$. We determine the spherically averaged BAO distance to $z = 1.52$ to 4.4 per cent precision: $D_V(z=1.52)=3855\pm170 \left(r_{\rm d}/r_{\rm d, fid}\right)\ $Mpc. This is the first time the location of the BAO feature has been measured between redshifts 1 and 2. Our result is fully consistent with the prediction obtained by extrapolating the Planck flat $\Lambda$CDM best-fit cosmology. All of our results are consistent with basic large-scale structure (LSS) theory, confirming quasars to be a reliable tracer of LSS, and provide a starting point for numerous cosmological tests to be performed with eBOSS quasar samples. We combine our result with previous, independent, BAO distance measurements to construct an updated BAO distance-ladder. Using these BAO data alone and marginalizing over the length of the standard ruler, we find $\Omega_{\Lambda} > 0$ at 6.5$\sigma$ significance when testing a $\Lambda$CDM model with free curvature.},
doi = {10.1093/mnras/stx2630},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 473,
place = {United States},
year = {Tue Jun 20 00:00:00 EDT 2017},
month = {Tue Jun 20 00:00:00 EDT 2017}
}

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