Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars
Abstract
We report a detection of the baryon acousticoscillation (BAO) feature in the flux-correlation function of the Lyα forest of high-redshift quasars with a statistical significance of five standard deviations. The study uses 137,562 quasars in the redshift range 2.1 ≤ z ≤ 3.5 from the data release 11 (DR11) of the Baryon Oscillation Spectroscopic Survey (BOSS) of SDSS-III. This sample contains three times the number of quasars used in previous studies. The measured position of the BAO peak determines the angular distance, DA(z = 2.34) and expansion rate, H(z = 2.34), both on a scale set by the sound horizon at the drag epoch, rd. We find DA/rd = 11.28 ± 0.65(1σ)$$+2.8\atop{-1.2}$$(2σ) and DH/rd = 9.18 ± 0.28(1σ) ± 0.6(2σ) where DH = c/H. The optimal combination, ~D$$0.7\atop{H}$$ D$0.3\atop{A}/rd is determined with a precision of ~2%. For the value rd = 147.4 Mpc, consistent with the cosmic microwave background power spectrum measured by Planck, we find DA(z = 2.34) = 1662 ± 96(1σ) Mpc and H(z = 2.34) = 222 ± 7(1σ) km s-1 Mpc-1. Tests with mock catalogs and variations of our analysis procedure have revealed no systematic uncertainties comparable to our statistical errors. Our results agree with the previously reported BAO measurement at the same redshift using the quasar-Lyα forest cross-correlation. The autocorrelation and cross-correlation approaches are complementary because of the quite different impact of redshift-space distortion on the two measurements. The combined constraints from the two correlation functions imply values of DA/rd that are 7% lower and 7% higher for DH/rd than the predictions of a flat ΛCDM cosmological model with the best-fit Planck parameters. With our estimated statistical errors, the significance of this discrepancy is ≈2.5σ.
- Authors:
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- Alternative Energies and Atomic Energy Commission (CEA), Saclay (France); Federal Inst. of Technology, Lausanne (Switzerland). Astrophysics Lab.
- CNRS/IN2P3. Univ. Paris (France). Observatoire de Paris. AstroParticule et Cosmologie (APC)
- CNRS/IN2P3. Univ. Paris (France). Observatoire de Paris. AstroParticule et Cosmologie (APC); Observatorio Nacional, Rio de Janeiro (Brazil); Institutional e-Astronomy Lab., Rio de Janeiro (Brazil)
- Alternative Energies and Atomic Energy Commission (CEA), Saclay (France)
- Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Max Planck Inst. for Astronomie, Heidelberg (Germany)
- Univ. of Portsmouth (United Kingdom). Inst. of Cosmology and Gravitation
- Inst. for Advanced Study, Princeton, NJ (United States)
- Apache Point Observatory, Sunspot, NM (United States)
- Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
- Harvard Univ., Cambridge, MA (United States). Harvard-Smithsonian Center for Astrophysics
- Univ of Barcelona, Barcelona (Spain). Inst. de Ciencies del Cosmos
- Federal Inst. of Technology, Lausanne (Switzerland). Astrophysics Lab.; Aix-Marseille Univ., and CNRS/LAM, Marseille (France)
- Catalan Inst. for Research and Advanced Studies, Barcelona, Catalonia (Spain); Univ of Barcelona, Barcelona (Spain). Inst. de Ciencies del Cosmos
- Univ. of Wyoming, Laramie, WY (United States). Dept. of Physics and Astronomy
- Univ. of Paris, Paris (France). Inst. d'Astrophysique de Paris
- Carnegie Mellon Univ., Pittsburgh, PA (United States). Bruce and Astrid McWilliams Center for Cosmology
- Univ. of Paris, Paris (France). Inst. d'Astrophysique de Paris
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Drexel Univ., Philadelphia, PA (United States). Dept. of Physics
- Alternative Energies and Atomic Energy Commission (CEA), Saclay (France); Sejong Univ., Seoul (Korea, Republic of). Dept. of Astronomy and Space Science
- Pennsylvania State Univ., University Park, PA (United States). Dept of Astronomy and Astrophysics; Pennsylvania State Univ., University Park, PA (United States). Inst. for Gravitation and the Cosmos
- The Ohio State Univ., Columbus, OH (United States). Dept. of Astronomy
- Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics and the Enrico Fermi Inst.
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1335435
- Report Number(s):
- BNL-112096-2016-JA
Journal ID: ISSN 0004-6361; KA2301020
- Grant/Contract Number:
- SC00112704; AC02-98CH10886; ANR-08-BLAN-0222; ANR-12- BS05-0015-01; PIIF-GA- 2011-301665
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Astronomy and Astrophysics
- Additional Journal Information:
- Journal Volume: 574; Journal ID: ISSN 0004-6361
- Publisher:
- EDP Sciences
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology; Lyα forest; large scale structure; dark energy
Citation Formats
Delubac, Timothée, Bautista, Julian E., Busca, Nicolás G., Rich, James, Kirkby, David, Bailey, Stephen, Font-Ribera, Andreu, Slosar, Anže, Lee, Khee-Gan, Pieri, Matthew M., Hamilton, Jean-Christophe, Aubourg, Éric, Blomqvist, Michael, Bovy, Jo, Brinkmann, Jon, Carithers, William, Dawson, Kyle S., Eisenstein, Daniel J., Gontcho A Gontcho, Satya, Kneib, Jean-Paul, Le Goff, Jean-Marc, Margala, Daniel, Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, O’Connell, Ross, Olmstead, Matthew D., Palanque-Delabrouille, Nathalie, Pâris, Isabelle, Petitjean, Patrick, Ross, Nicholas P., Rossi, Graziano, Schlegel, David J., Schneider, Donald P., Weinberg, David H., Yèche, Christophe, and York, Donald G. Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars. United States: N. p., 2015.
Web. doi:10.1051/0004-6361/201423969.
Delubac, Timothée, Bautista, Julian E., Busca, Nicolás G., Rich, James, Kirkby, David, Bailey, Stephen, Font-Ribera, Andreu, Slosar, Anže, Lee, Khee-Gan, Pieri, Matthew M., Hamilton, Jean-Christophe, Aubourg, Éric, Blomqvist, Michael, Bovy, Jo, Brinkmann, Jon, Carithers, William, Dawson, Kyle S., Eisenstein, Daniel J., Gontcho A Gontcho, Satya, Kneib, Jean-Paul, Le Goff, Jean-Marc, Margala, Daniel, Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, O’Connell, Ross, Olmstead, Matthew D., Palanque-Delabrouille, Nathalie, Pâris, Isabelle, Petitjean, Patrick, Ross, Nicholas P., Rossi, Graziano, Schlegel, David J., Schneider, Donald P., Weinberg, David H., Yèche, Christophe, & York, Donald G. Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars. United States. https://doi.org/10.1051/0004-6361/201423969
Delubac, Timothée, Bautista, Julian E., Busca, Nicolás G., Rich, James, Kirkby, David, Bailey, Stephen, Font-Ribera, Andreu, Slosar, Anže, Lee, Khee-Gan, Pieri, Matthew M., Hamilton, Jean-Christophe, Aubourg, Éric, Blomqvist, Michael, Bovy, Jo, Brinkmann, Jon, Carithers, William, Dawson, Kyle S., Eisenstein, Daniel J., Gontcho A Gontcho, Satya, Kneib, Jean-Paul, Le Goff, Jean-Marc, Margala, Daniel, Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, O’Connell, Ross, Olmstead, Matthew D., Palanque-Delabrouille, Nathalie, Pâris, Isabelle, Petitjean, Patrick, Ross, Nicholas P., Rossi, Graziano, Schlegel, David J., Schneider, Donald P., Weinberg, David H., Yèche, Christophe, and York, Donald G. Mon .
"Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars". United States. https://doi.org/10.1051/0004-6361/201423969. https://www.osti.gov/servlets/purl/1335435.
@article{osti_1335435,
title = {Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars},
author = {Delubac, Timothée and Bautista, Julian E. and Busca, Nicolás G. and Rich, James and Kirkby, David and Bailey, Stephen and Font-Ribera, Andreu and Slosar, Anže and Lee, Khee-Gan and Pieri, Matthew M. and Hamilton, Jean-Christophe and Aubourg, Éric and Blomqvist, Michael and Bovy, Jo and Brinkmann, Jon and Carithers, William and Dawson, Kyle S. and Eisenstein, Daniel J. and Gontcho A Gontcho, Satya and Kneib, Jean-Paul and Le Goff, Jean-Marc and Margala, Daniel and Miralda-Escudé, Jordi and Myers, Adam D. and Nichol, Robert C. and Noterdaeme, Pasquier and O’Connell, Ross and Olmstead, Matthew D. and Palanque-Delabrouille, Nathalie and Pâris, Isabelle and Petitjean, Patrick and Ross, Nicholas P. and Rossi, Graziano and Schlegel, David J. and Schneider, Donald P. and Weinberg, David H. and Yèche, Christophe and York, Donald G.},
abstractNote = {We report a detection of the baryon acousticoscillation (BAO) feature in the flux-correlation function of the Lyα forest of high-redshift quasars with a statistical significance of five standard deviations. The study uses 137,562 quasars in the redshift range 2.1 ≤ z ≤ 3.5 from the data release 11 (DR11) of the Baryon Oscillation Spectroscopic Survey (BOSS) of SDSS-III. This sample contains three times the number of quasars used in previous studies. The measured position of the BAO peak determines the angular distance, DA(z = 2.34) and expansion rate, H(z = 2.34), both on a scale set by the sound horizon at the drag epoch, rd. We find DA/rd = 11.28 ± 0.65(1σ)$+2.8\atop{-1.2}$(2σ) and DH/rd = 9.18 ± 0.28(1σ) ± 0.6(2σ) where DH = c/H. The optimal combination, ~D$0.7\atop{H}$ D$0.3\atop{A}/rd is determined with a precision of ~2%. For the value rd = 147.4 Mpc, consistent with the cosmic microwave background power spectrum measured by Planck, we find DA(z = 2.34) = 1662 ± 96(1σ) Mpc and H(z = 2.34) = 222 ± 7(1σ) km s-1 Mpc-1. Tests with mock catalogs and variations of our analysis procedure have revealed no systematic uncertainties comparable to our statistical errors. Our results agree with the previously reported BAO measurement at the same redshift using the quasar-Lyα forest cross-correlation. The autocorrelation and cross-correlation approaches are complementary because of the quite different impact of redshift-space distortion on the two measurements. The combined constraints from the two correlation functions imply values of DA/rd that are 7% lower and 7% higher for DH/rd than the predictions of a flat ΛCDM cosmological model with the best-fit Planck parameters. With our estimated statistical errors, the significance of this discrepancy is ≈2.5σ.},
doi = {10.1051/0004-6361/201423969},
journal = {Astronomy and Astrophysics},
number = ,
volume = 574,
place = {United States},
year = {Mon Jan 26 00:00:00 EST 2015},
month = {Mon Jan 26 00:00:00 EST 2015}
}
Web of Science
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