The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
Abstract
We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameter H from the baryon acoustic oscillation (BAO) method, in combination with a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvaturemore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- SDSS-III Collaboration
- OSTI Identifier:
- 1324267
- Alternate Identifier(s):
- OSTI ID: 1379928; OSTI ID: 1594736
- Report Number(s):
- BNL-112527-2016-JA
Journal ID: ISSN 0035-8711; KA2301020
- Grant/Contract Number:
- SC0012704; SC0014329; SC0010331; SC0009959; SC0013718; ST/M001709/1; ST/N000668/1; ST/K004719/1; ST/N00180X/1; AC02-05CH11231; SC0017860
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 470; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; distance scale; large-scale structure
Citation Formats
Alam, Shadab, Ata, Metin, Bailey, Stephen, Beutler, Florian, Bizyaev, Dmitry, Blazek, Jonathan A., Bolton, Adam S., Brownstein, Joel R., Burden, Angela, Chuang, Chia-Hsun, Comparat, Johan, Cuesta, Antonio J., Dawson, Kyle S., Eisenstein, Daniel J., Escoffier, Stephanie, Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Ho, Shirley, Kinemuchi, Karen, Kirkby, David, Kitaura, Francisco, Malanushenko, Elena, Malanushenko, Viktor, Maraston, Claudia, McBride, Cameron K., Nichol, Robert C., Olmstead, Matthew D., Oravetz, Daniel, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Price-Whelan, Adrian M., Reid, Beth A., Rodríguez-Torres, Sergio A., Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Saito, Shun, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Scóccola, Claudia G., Seo, Hee-Jong, Sheldon, Erin S., Simmons, Audrey, Slosar, Anže, Strauss, Michael A., Swanson, Molly E. C., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Magaña, Mariana Vargas, Vazquez, Jose Alberto, Verde, Licia, Wake, David A., Wang, Yuting, Weinberg, David H., White, Martin, Wood-Vasey, W. Michael, Yèche, Christophe, Zehavi, Idit, Zhai, Zhongxu, and Zhao, Gong-Bo. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. United States: N. p., 2017.
Web. doi:10.1093/mnras/stx721.
Alam, Shadab, Ata, Metin, Bailey, Stephen, Beutler, Florian, Bizyaev, Dmitry, Blazek, Jonathan A., Bolton, Adam S., Brownstein, Joel R., Burden, Angela, Chuang, Chia-Hsun, Comparat, Johan, Cuesta, Antonio J., Dawson, Kyle S., Eisenstein, Daniel J., Escoffier, Stephanie, Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Ho, Shirley, Kinemuchi, Karen, Kirkby, David, Kitaura, Francisco, Malanushenko, Elena, Malanushenko, Viktor, Maraston, Claudia, McBride, Cameron K., Nichol, Robert C., Olmstead, Matthew D., Oravetz, Daniel, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Price-Whelan, Adrian M., Reid, Beth A., Rodríguez-Torres, Sergio A., Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Saito, Shun, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Scóccola, Claudia G., Seo, Hee-Jong, Sheldon, Erin S., Simmons, Audrey, Slosar, Anže, Strauss, Michael A., Swanson, Molly E. C., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Magaña, Mariana Vargas, Vazquez, Jose Alberto, Verde, Licia, Wake, David A., Wang, Yuting, Weinberg, David H., White, Martin, Wood-Vasey, W. Michael, Yèche, Christophe, Zehavi, Idit, Zhai, Zhongxu, & Zhao, Gong-Bo. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. United States. https://doi.org/10.1093/mnras/stx721
Alam, Shadab, Ata, Metin, Bailey, Stephen, Beutler, Florian, Bizyaev, Dmitry, Blazek, Jonathan A., Bolton, Adam S., Brownstein, Joel R., Burden, Angela, Chuang, Chia-Hsun, Comparat, Johan, Cuesta, Antonio J., Dawson, Kyle S., Eisenstein, Daniel J., Escoffier, Stephanie, Gil-Marín, Héctor, Grieb, Jan Niklas, Hand, Nick, Ho, Shirley, Kinemuchi, Karen, Kirkby, David, Kitaura, Francisco, Malanushenko, Elena, Malanushenko, Viktor, Maraston, Claudia, McBride, Cameron K., Nichol, Robert C., Olmstead, Matthew D., Oravetz, Daniel, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Prada, Francisco, Price-Whelan, Adrian M., Reid, Beth A., Rodríguez-Torres, Sergio A., Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Saito, Shun, Salazar-Albornoz, Salvador, Samushia, Lado, Sánchez, Ariel G., Satpathy, Siddharth, Schlegel, David J., Schneider, Donald P., Scóccola, Claudia G., Seo, Hee-Jong, Sheldon, Erin S., Simmons, Audrey, Slosar, Anže, Strauss, Michael A., Swanson, Molly E. C., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Magaña, Mariana Vargas, Vazquez, Jose Alberto, Verde, Licia, Wake, David A., Wang, Yuting, Weinberg, David H., White, Martin, Wood-Vasey, W. Michael, Yèche, Christophe, Zehavi, Idit, Zhai, Zhongxu, and Zhao, Gong-Bo. Tue .
"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample". United States. https://doi.org/10.1093/mnras/stx721. https://www.osti.gov/servlets/purl/1324267.
@article{osti_1324267,
title = {The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample},
author = {Alam, Shadab and Ata, Metin and Bailey, Stephen and Beutler, Florian and Bizyaev, Dmitry and Blazek, Jonathan A. and Bolton, Adam S. and Brownstein, Joel R. and Burden, Angela and Chuang, Chia-Hsun and Comparat, Johan and Cuesta, Antonio J. and Dawson, Kyle S. and Eisenstein, Daniel J. and Escoffier, Stephanie and Gil-Marín, Héctor and Grieb, Jan Niklas and Hand, Nick and Ho, Shirley and Kinemuchi, Karen and Kirkby, David and Kitaura, Francisco and Malanushenko, Elena and Malanushenko, Viktor and Maraston, Claudia and McBride, Cameron K. and Nichol, Robert C. and Olmstead, Matthew D. and Oravetz, Daniel and Padmanabhan, Nikhil and Palanque-Delabrouille, Nathalie and Pan, Kaike and Pellejero-Ibanez, Marcos and Percival, Will J. and Petitjean, Patrick and Prada, Francisco and Price-Whelan, Adrian M. and Reid, Beth A. and Rodríguez-Torres, Sergio A. and Roe, Natalie A. and Ross, Ashley J. and Ross, Nicholas P. and Rossi, Graziano and Rubiño-Martín, Jose Alberto and Saito, Shun and Salazar-Albornoz, Salvador and Samushia, Lado and Sánchez, Ariel G. and Satpathy, Siddharth and Schlegel, David J. and Schneider, Donald P. and Scóccola, Claudia G. and Seo, Hee-Jong and Sheldon, Erin S. and Simmons, Audrey and Slosar, Anže and Strauss, Michael A. and Swanson, Molly E. C. and Thomas, Daniel and Tinker, Jeremy L. and Tojeiro, Rita and Magaña, Mariana Vargas and Vazquez, Jose Alberto and Verde, Licia and Wake, David A. and Wang, Yuting and Weinberg, David H. and White, Martin and Wood-Vasey, W. Michael and Yèche, Christophe and Zehavi, Idit and Zhai, Zhongxu and Zhao, Gong-Bo},
abstractNote = {We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameter H from the baryon acoustic oscillation (BAO) method, in combination with a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature ΩK = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter w = -1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H0 = 67.3 ± 1.0 km s-1 Mpc-1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H0 = 67.8 ± 1.2 km s-1 Mpc-1. Assuming flat ΛCDM, we find Ωm = 0.310 ± 0.005 and H0 = 67.6 ± 0.5 km s-1 Mpc-1, and we find a 95 per cent upper limit of 0.16 eV c-2 on the neutrino mass sum.},
doi = {10.1093/mnras/stx721},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 470,
place = {United States},
year = {Tue Mar 28 00:00:00 EDT 2017},
month = {Tue Mar 28 00:00:00 EDT 2017}
}
Web of Science
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