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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 1.

The close relationship between the number counts of each 3D-Herschel field (binned by flux) demonstrates that the photometric estimations were consistent across all fields. Error bars are determined as the fraction error of each bin (﹩1/\sqrt{N}\times N\,{\rm{d}}{\rm{e}}{{\rm{x}}}^{-1}\,{\rm{d}}{\rm{e}}{{\rm{g}}}^{-2}﹩).

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