Figure 1 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 1.

g − i color–mass distributions of the three different target classes utilized in this paper. The color contours represent the CMASS galaxy sample, with color representing density of points in each cell. The black curves represent the density contours of SPARSE targets. The WISE targets are sparse enough that they can be shown individually, represented by the filled circles. All results are shown in the redshift range of ﹩z=[0.45,0.60]﹩.

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