The DOI matches its Crossref record; 13 of the 13 references it cites were found in a registry or an index.
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
Open accessAbstract
We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey, which is part of the Sloan Digital Sky Survey III.Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately 8500 square degrees and the redshift range 0.2 < z < 0.7.We also compare these results with those from the publicly released DR9 and DR10 samples.Assuming a concordance cold dark matter ( CDM) cosmological model, the DR11 sample covers a volume of 13 Gpc 3 and is the largest region of the Universe ever surveyed at this density.We measure the correlation function and power spectrum, including density-field reconstruction of the BAO feature.The acoustic features are detected at a significance of over 7σ in both the correlation function and power spectrum.Fitting for the position of the acoustic features measures the distance relative to the sound horizon at the drag epoch, r d , which has a value of r d,fid = 149.28Mpc in our fiducial cosmology.We find D V = (1264 ± 25 Mpc)(r d /r d,fid ) Hubble Fellow.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
Self-citationTHE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
Self-citationLewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
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 2×
“C© 2012 The Authors, MNRAS 427, 3435–3467 Monthly Notices of the Royal Astronomical Society C© 2012 RAS at C arnegie M ellon U niversity on M arch 2, 2016 http://m nras.oxfordjournals.org/ D ow nloaded from We follow the methodology in Mehta et al. (2012), using the CosmoMC (Lewis & Bridle 2002) Markov Chain Monte Car…”
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 · cited 1×
“A drift-scanning mosaic CCD camera (Gunn et al. 1998) imaged the sky in five photometric bandpasses (Fukugita et al. 1996; Smith et al. 2002; Doi et al. 2010) to a limiting magnitude of r 22.5.”
MethodInfluentialSelf-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 5×
“Our BAO distance constraints are parametrized as described above as a measurement on DV/rs at z = 0.57; we augment these with the z = 0.35 measurement from Padmanabhan et al. (2012a) as well as the 6dF measurement at z = 0.106 (Beutler et al. 2011).”
BackgroundMethodInfluentialSelf-citationBaryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample
Percival, W. J., Reid, B. A., Eisenstein, D. J., Bahcall, N. A., Budavari, T., Frieman, J. A., Fukugita, M., Gunn, J. E., Ivezić, Ž., Knapp, G. R., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15812.x · Cited by 1,846 · cited 14×
“The galaxy target selection in BOSS is divided into two classes of galaxies: LOWZ galaxies (0.2 z 0.43) and CMASS galaxies (0.43 z 0.7), analogous to the Cut-I and II SDSS-II LRGs.”
MethodResultInfluentialSelf-citationThe 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-citation
Cited by
Dark Matter as a Topological Vacuum Condensate
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1807.06209 · Cited by 3,403
Self-citationAlam, 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-citationThe clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15
Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv154 · Cited by 1,745
“…and then summed into 8 h−1Mpc bins, allowing different choices for bin centres . c© 2014 RAS, MNRAS 000, 1–13 We measure the spherically-averaged power spectrum, P (k), using the standard Fourier technique of Feldman et al. (1994), as described in Reid et al. (2010) and Anderson et al. (2012).”
BackgroundMethodSelf-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
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023520 · Cited by 1,124
Self-citation
Metadata
- Authors
- Anderson, L., Aubourg, É., Bailey, S., Beutler, F., Bhardwaj, V., Blanton, M., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Burden, A., Chuang, C.-H., Cuesta, A. J., Dawson, K. S., Eisenstein, D. J., Escoffier, S., Gunn, J. E., Guo, H., Ho, S., Honscheid, K., Howlett, C., Kirkby, D., Lupton, R. H., Manera, M., Maraston, C., McBride, C. K., Mena, O., Montesano, F., Nichol, R. C., Nuza, S. E., Olmstead, M. D., Padmanabhan, N., Palanque-Delabrouille, N., Parejko, J., Percival, W. J., Petitjean, P., Prada, F., Price-Whelan, A. M., Reid, B., Roe, N. A., Ross, A. J., Ross, N. P., Sabiu, C. G., Saito, S., Samushia, L., Sánchez, A. G., Schlegel, D. J., Schneider, D. P., Scoccola, C. G., Seo, H.-J., Skibba, R. A., Strauss, M. A., Swanson, M. E. C., Thomas, D., Tinker, J. L., Tojeiro, R., Magaña, M. V., Verde, L., Wake, D. A., Weaver, B. A., Weinberg, D. H., White, M., Xu, X., Yèche, C., Zehavi, I., & Zhao, G.-B.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2014-04-21
- Volume
- 441
- Issue
- 1
- Pages
- 24-62
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2156305595
- Cited by
- 1,842
- References
- 13
- FWCI
- 135.14
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples. https://app.cochat.ai/papers/10.1093/mnras/stu523
- The paper
- Anderson, L., Aubourg, É., Bailey, S., Beutler, F., Bhardwaj, V., Blanton, M., Bolton, A. S., Brinkmann, J., Brownstein, J. R., Burden, A., Chuang, C.-H., Cuesta, A. J., Dawson, K. S., Eisenstein, D. J., Escoffier, S., Gunn, J. E., Guo, H., Ho, S., Honscheid, K., . . . Zhao, G.-B. (2014). The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stu523
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.