Figure 2 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 2.

Diagram summarizing the procedures for generating the star-forming galaxies at z ≳ 4. ﹩{M}_{\star }﹩ is defined as ﹩\mathrm{log}(M/{M}_{\odot })﹩. Gray boxes indicate the empirical relationships, distributions, or data on which mock galaxy properties are based, and colored boxes indicate the mock galaxy property generated in that step. All star-forming mock galaxies at z > 4 are generated following these procedures. Quiescent galaxies are generated at z > 4 following a different procedure, which is described in Section 4 and illustrated in Figure 13.

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