{"paper":{"title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam S. Bolton, Adrian M. Price-Whelan, Angela Burden, Antonio J. Cuesta, Ariel G. Sanchez, Ashley J. Ross, Benjamin A. Weaver, Beth Reid, Cameron K. McBride, Chia-Hsun Chuang, Christophe Yeche, Claudia G. Scoccola, Claudia Maraston, Cristiano G. Sabiu, Cullan Howlett, Daniel J. Eisenstein, Daniel Thomas, David A. Wake, David H. Weinberg, David J. Schlegel, David Kirkby, Donald P. Schneider, Eric Aubourg, Florian Beutler, Francesco Montesano, Francisco Prada, Gong-Bo Zhao, Hee-Jong Seo, Hong Guo, Idit Zehavi, James E. Gunn, J. Brinkmann, Jeremy L. Tinker, Joel R. Brownstein, John Parejko, Klaus Honscheid, Kyle S. Dawson, Lado Samushia, Lauren Anderson, Licia Verde, Marc Manera, Mariana Vargas Magana, Martin White, Matthew D. Olmstead, Michael A. Strauss, Michael Blanton, Molly E. C. Swanson, Natalie A. Roe, Nathalie Palanque-Delabrouille, Nicholas P. Ross, Nikhil Padmanabhan, Olga Mena, Patrick Petitjean, Ramin A. Skibba, Rita Tojeiro, Robert C. Nichol, Robert H. Lupton, Sebastian E. Nuza, Shirley Ho, Shun Saito, Stephanie Escoffier, Stephen Bailey, Vaishali Bhardwaj, Will J. Percival, Xiaoying Xu","submitted_at":"2013-12-17T17:49:44Z","abstract_excerpt":"We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III). Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately $8\\,500$ 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 $\\Lambda$CDM cosmological model,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.4877","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}