Figure 4 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 4.

Upper panel: the total BOSS stellar mass function at ﹩z=[0.45,0.60]﹩, down to our completeness limit of ﹩\mathrm{log}{M}_{* }=11.4﹩. The best-fit parameters of equation (x) are shown with the solid curve. Lower panel: residuals of the fit. The y-axis is ﹩({{\rm{\Phi }}}_{\mathrm{BOSS}}-{{\rm{\Phi }}}_{\mathrm{fit}})/{{\rm{\Phi }}}_{\mathrm{fit}}﹩. The ﹩{\chi }^{2}﹩ for this fit is 7.0 for (10–5) degrees of freedom.

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