The Correlation between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe

The Correlation between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe

We present measurements of the clustering of galaxies as a function of their stellar mass in the Baryon Oscillation Spectroscopic Survey. We compare the clustering of samples using 12 different methods for estimating stellar mass, isolating the method that has the smallest scatter at fixed halo mass...

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Bibliographic Details
Main Authors: Tinker, Jeremy L., Brownstein, Joel R., Guo, Hong, Leauthaud, Alexie, Maraston, Claudia, Masters, Karen, Montero-Dorta, Antonio D., Thomas, Daniel, Tojeiro, Rita, Weiner, Benjamin, Zehavi, Idit, Olmstead, Matthew D.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
cosmology: observations
galaxies: abundances
galaxies: evolution
galaxies: halos
galaxies: luminosity function
mass function
Online Access:http://hdl.handle.net/10150/624043
http://arizona.openrepository.com/arizona/handle/10150/624043

Internet

http://hdl.handle.net/10150/624043
http://arizona.openrepository.com/arizona/handle/10150/624043

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