Figure 10 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 10.

UV continuum slopes predicted by the spectral evolution model adopted in this work. We show model predictions for a constant SFH of different ages and three metallicities: ﹩\mathrm{log}Z/{Z}_{\odot }=-2﹩ (blue), −1 (green), and 0 (orange). Dashed lines indicate predictions for stellar emission only, while solid lines for stellar and nebular continuum emission. In this latter case, we consider a photoionization model with ionization parameter ﹩\mathrm{log}{U}_{{\rm{S}}}=-2.5﹩ and depletion factor ﹩{\xi }_{{\rm{d}}}=0.3﹩.

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