Figure 7 from The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History

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The JWST Extragalactic Mock Catalog: Modeling Galaxy Populations from the UV through the Near-IR over 13 Billion Years of Cosmic History

Authors: Christina C. Williams, Emma Curtis-Lake, Kevin N. Hainline, Jacopo Chevallard, Brant E. Robertson, Stephane Charlot, Ryan Endsley, Daniel P. Stark, Christopher N. A. Willmer, Stacey Alberts, Ricardo Amorin, Santiago Arribas, Stefi Baum, Andrew Bunker, Stefano Carniani, Sara Crandall, Eiichi Egami, Daniel J. Eisenstein, Bernd Husemann, Michael V. Maseda, Roberto Maiolino, Timothy D. Rawle, Marcia Rieke, Renske Smit, Sandro Tacchella, and Chris J. Willott

2018 The Astrophysical Journal Supplement Series 236 33.

Provider: AAS Journals

Caption: Figure 7.

The redshift evolution of the intercept of the ﹩{M}_{{\rm{UV}}}﹩–﹩{M}_{\star }﹩ distribution, ﹩{M}_{{\rm{UV}}-{M}_{\star }}^{0}(z)﹩, defined at ﹩{M}_{{\rm{UV}}}=-20﹩. Blue points indicate the best-fit intercept to the 3D-HST data presented in Figure 6, assuming a fixed slope. Error bars are smaller than the size of the symbol. Orange points are based on the relation presented in Stark et al. (2013) that includes the correction for nebular emission lines.

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