The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modelling the clustering and halo occupation distribution of BOSS CMASS galaxies in the Final Data Release

By Sergio A. Rodr'iguez-Torres, C. Chuang, Francisco Prada, Hong Guo, Anatoly Klypin, P. Behroozi, C. Hahn, J. Comparat, G. Yepes, A. Montero-Dorta and 14 more. 2015

160 citations recorded by the source corpus.

Citation: Rodriguez-Torres, S. A., Chuang, C. H., Prada, F., Guo, H., Klypin, A., Behroozi, P., . . . Thomas, D. (2016). The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modelling the clustering and halo occupation distribution of BOSS CMASS galaxies in the Final Data Release. Monthly Notices of the Royal Astronomical Society, 460(2), 1173-1187. doi:10.1093/mnras/stw1014

Subfields: Astronomy and Astrophysics, Ecology, Instrumentation

View Paper: https://www.semanticscholar.org/paper/c0481509e888957e7b400450929c8ad27b7c3241

How researchers see this paper

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In Astronomy and Astrophysics

1. D. Schneider
2. Will J. Percival
3. Daniel J. Eisenstein
4. C. Chuang
5. J. Brownstein
6. P. Hopkins
7. L. Hernquist
8. A. Ross

In Ecology

1. Will J. Percival
2. D. Schneider
3. J. Newman
4. Risa Wechsler
5. Daniel J. Eisenstein
6. John Moustakas
7. David Schlegel
8. Adam D. Myers

In Instrumentation

1. D. Schneider
2. Will J. Percival
3. Daniel J. Eisenstein
4. J. Brownstein
5. C. Chuang
6. C. Conroy
7. Risa Wechsler
8. A. Ross

Citations in the corpus

• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering (2013, methodology): “These mock catalogues were constructed using a similar procedure described in Rodriguez-Torres et al. 2016 where they constructed the BOSS DR12 lightcone mock catalogues using the MultiDark N-body simulations (Klypin et al. 2016).”
• Target Selection and Validation of DESI Luminous Red Galaxies (2022, background): “…& Mandelbaum 2015; Zhou et al. 2021) and study galaxy–galaxy lensing (e.g., Alam et al. 2017; Jullo et al. 2019), halo occupation distribution (e.g., Rodríguez-Torres et al. 2016), and evolution of the most massive galaxies (e.g., Bundy et al. 2017), it is desirable to have a large spectroscopic…”
• Combining full-shape and BAO analyses of galaxy power spectra: a 1.6% CMB-independent constraint on H0 (2020, methodology): “Halo abundance matching [92] is used to ensure the simulations have the correct redshift evolution and correlation functions, and separate mocks are produced for each of the four BOSS DR12 chunks (section 3.”
• Cosmological parameters from the BOSS galaxy power spectrum (2019, background): “The halo bias is in general different from galaxy bias, but given that the satellite fraction is relatively small in the BOSS samples [74], we expect these estimates not”