The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring growth rate and geometry with anisotropic clustering
Open accessAbstract
We use the observed anisotropic clustering of galaxies in the Baryon Oscillation Spectroscopic Survey Data Release 11 CMASS sample to measure the linear growth rate of structure, the Hubble expansion rate and the comoving distance scale. Our sample covers 8498 deg2 and encloses an effective volume of 6 Gpc3 at an effective redshift of |$\bar{z} = 0.57$|. We find fσ8 = 0.441 ± 0.044, H = 93.1 ± 3.0 km s−1 Mpc−1 and DA = 1380 ± 23 Mpc when fitting the growth and expansion rate simultaneously. When we fix the background expansion to the one predicted by spatially flat Λ cold dark matter (ΛCDM) model in agreement with recent Planck results, we find fσ8 = 0.447 ± 0.028 (6 per cent accuracy). While our measurements are generally consistent with the predictions of ΛCDM and general relativity, they mildly favour models in which the strength of gravitational interactions is weaker than what is predicted by general relativity. Combining our measurements with recent cosmic microwave background data results in tight constraints on basic cosmological parameters and deviations from the standard cosmological model. Separately varying these parameters, we find w = −0.983 ± 0.075 (8 per cent accuracy) and γ = 0.69 ± 0.11 (16 per cent accuracy) for the effective equation of state of dark energy and the growth rate index, respectively. Both constraints are in good agreement with the standard model values of w = −1 and γ = 0.554.
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Cites
Cosmological parameters from CMB and other data: A Monte Carlo approach
Lewis, A., & Bridle, S. (2002) · Physical Review D · doi:10.1103/physrevd.66.103511 · Cited by 3,495 · cited 1×
“To sample cosmological parameter space, we use the Monte Carlo Markov Chain (MCMC) technique implemented by the COSMOMC package (Lewis & Bridle 2002).”
MethodThe Sloan Digital Sky Survey Photometric System
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. (1996) · The Astronomical Journal · doi:10.1086/117915 · Cited by 3,033
Self-citationBeutler, F., Blake, C., Colless, M., Jones, D. H., Staveley-Smith, L., Campbell, L., Parker, Q., Saunders, W., & Watson, F. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19250.x · Cited by 2,590 · cited 1×
“Recent highlights include the BAO measurements from the 6dF Galaxy Redshift Survey (6dFGRS; Beutler et al. 2011), Sloan Digital Sky Survey II (SDSS-II; Padmanabhan et al. 2012), SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 9 sample (DR9; Anderson et al. 2012), WiggleZ survey…”
MethodSelf-citationExploring the Expansion History of the Universe
Linder, E. V. (2003) · Physical Review Letters · doi:10.1103/physrevlett.90.091301 · Cited by 2,526
The Sloan Digital Sky Survey Photometric Camera
Gunn, J. E., Carr, M., Rockosi, C., Sekiguchi, M., Berry, K., Elms, B., de Haas, E., Ivezić, Ž., Knapp, G., Lupton, R., et al. (1998) · The Astronomical Journal · doi:10.1086/300645 · Cited by 1,692
Self-citationA test of the nature of cosmic acceleration using galaxy redshift distortions
Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Le Fèvre, O., Marinoni, C., Garilli, B., Blaizot, J., De Lucia, G., Pollo, A., et al. (2008) · Nature · doi:10.1038/nature06555 · Cited by 654
Cited by
Alam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx721 · Cited by 3,056
Self-citationBeyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
Hildebrandt, H., Viola, M., Heymans, C., Joudaki, S., Kuijken, K., Blake, C., Erben, T., Joachimi, B., Klaes, D., Miller, L., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2805 · Cited by 1,021
Desjacques, V., Jeong, D., & Schmidt, F. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.12.002 · Cited by 817
Planck 2015 results: XIV. Dark energy and modified gravity
Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201525814 · Cited by 699
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Metadata
- Authors
- Samushia, L., Reid, B. A., White, M., Percival, W. J., Cuesta, A. J., Zhao, G.-B., Ross, A. J., Manera, M., Aubourg, É., Beutler, F., Brinkmann, J., Brownstein, J. R., Dawson, K. S., Eisenstein, D. J., Ho, S., Honscheid, K., Maraston, C., Montesano, F., Nichol, R. C., Roe, N. A., Ross, N. P., Sánchez, A. G., Schlegel, D. J., Schneider, D. P., Streblyanska, A., Thomas, D., Tinker, J. L., Wake, D. A., Weaver, B. A., & Zehavi, I.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2014-02-27
- Volume
- 439
- Issue
- 4
- Pages
- 3504-3519
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2065889919
- Cited by
- 269
- References
- 6
- FWCI
- 30.92
- Type
- journal article
- Language
- en
- Open access
- bronze
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- The paper
- Samushia, L., Reid, B. A., White, M., Percival, W. J., Cuesta, A. J., Zhao, G.-B., Ross, A. J., Manera, M., Aubourg, É., Beutler, F., Brinkmann, J., Brownstein, J. R., Dawson, K. S., Eisenstein, D. J., Ho, S., Honscheid, K., Maraston, C., Montesano, F., Nichol, R. C., . . . Zehavi, I. (2014). The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring growth rate and geometry with anisotropic clustering. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stu197
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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