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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 9.

Characteristic dust temperature (Td,char; Equation (3)) as a function of redshift for the IR-bright sample. Points are color-coded by ﹩{U}_{{\rm{\min }}}﹩, with its distribution shown as a histogram along the color bar. Median reference lines mark the fixed ﹩{U}_{{\rm{\min }}}﹩ fits (dashed navy; 18.4 K), the full 3D-Herschel mass-limited sample (black; 25.4 ± 2.1 K), and the IR-bright subsample (red; 25.7 ± 3.3 K).

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