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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 A2.

Distributions of uncertainty-normalized flux residuals (Equation (A1)) for each field and instrument. Left column: PACS bands; right column: SPIRE bands. Rows correspond to GOODS-S, GOODS-N, COSMOS, and UDS from top to bottom. The dashed curve shows the unit Gaussian ﹩{ \mathcal N }(0,1)﹩ expected for perfectly Gaussian, well-calibrated uncertainties. The comparison catalog used in each panel is indicated in the upper right. The fractions f1σ and f2σ give the fraction of sources with ∣ΔF/σΔF∣ within 1 and 2, respectively.

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