Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 447, Issue 1, Pages 437-445Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu2465
Keywords
galaxies: haloes; galaxies: statistics; large-scale structure of Universe
Categories
Funding
- European Research Council
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- University of Cambridge
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
- Science and Technology Facilities Council [ST/J005673/1, ST/J500665/1, ST/K502248/1, 1246657, ST/K00090X/1, ST/K00333X/1] Funding Source: researchfish
- STFC [ST/J500665/1, ST/J005673/1, ST/K004719/1, ST/K00090X/1, ST/K00333X/1, ST/J001511/1, ST/K502248/1] Funding Source: UKRI
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We present 1000 mock galaxy catalogues (mocks) for the analysis of the low-redshift sample (LOWZ; effective redshift z similar to 0.32) of the Baryon Oscillation Spectroscopic Survey (BOSS) Data Releases 10 and 11. These mocks have been created following the PTHalos method revised to include new developments. The main improvement is the introduction of a redshift dependence in the halo occupation distribution in order to account for the change of the galaxy number density with redshift. These mock galaxy catalogues are used in the analyses of the LOWZ galaxy clustering by the BOSS collaboration.
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