Figure 8 from The Correlation between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe

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

Authors: Jeremy L. Tinker, Joel R. Brownstein, Hong Guo, Alexie Leauthaud, Claudia Maraston, Karen Masters, Antonio D. Montero-Dorta, Daniel Thomas, Rita Tojeiro, Benjamin Weiner, Idit Zehavi, and Matthew D. Olmstead

2017 The Astrophysical Journal 839 121.

Provider: AAS Journals

Caption: Figure 8.

The combined CMASS+SPARSE bias values compared with models derived by abundance matching dark matter halos and subhalos in the MultiDark simulation and the stellar mass function of BOSS. Different curves indicate different values of scatter (in ﹩\mathrm{log}{M}_{* }﹩) in stellar mass at fixed halo mass.

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