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The clustering of galaxies in the sdss-iii baryon oscillation spectroscopic survey: The low-redshift sample
John K. Parejko, Tomomi Sunayama, Nikhil Padmanabhan, David A. Wake, Andreas A. Berlind, Dmitry Bizyaev, Michael Blanton, Adam S. Bolton, Frank van den Bosch, Jon Brinkmann, Joel R. Brownstein, Luiz Alberto Nicolaci da Costa, Daniel J. Eisenstein, Hong Guo, Eyal Kazin, Marcio Maia, Elena Malanushenko, Claudia Maraston, Cameron K. McBride, Robert C. Nichol, Daniel J. Oravetz, Kaike Pan, Will J. Percival, Francisco Prada, Ashley J. Ross, Nicholas P. Ross, David J. Schlegel, Don Schneider, Audrey E. Simmons, Ramin Skibba, Jeremy Tinker, Rita Tojeiro, Benjamin A. Weaver, Andrew Wetzel, Martin White, David H. Weinberg, Daniel Thomas, Idit Zehavi & Zheng Zheng
Abstract
We report on the small-scale (0.5 13 h - 1M, a large-scale bias of ~2.0 and a satellite fraction of 12 ± 2 per cent. Thus, these galaxies occupy haloes with average masses in between those of the higher redshift BOSS CMASS sample and the original SDSS I/II luminous red galaxy sample © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society © doi:10.1093/mnras/sts314.Links
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