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3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies

  • Authors: Seamus McNulty, Mimi Song, Katherine E. Whitaker, Joel Leja, Aubrey Medrano, Elijah P. Mathews, Mark Dickinson, Hanae Inami, Ivo Labbe, Danilo Marchesini, Alexandra Pope, Irene Shivaei

Seamus McNulty et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 2.

Comparison of posterior medians inferred from full Prospector fits of the adjusted 3D-HST catalog (J. Leja et al. 2019b; x-axis) versus our Prospector emulation on the publicly released 3D-HST catalog (y-axis). Panels show (top) stellar mass, (middle) SFR, and (bottom) diffuse dust attenuation. The one-to-one line is in black, and red lines show median offsets. The emulator reproduces direct-fit estimates within their statistical uncertainties.

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