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Everything Every Band All at Once. I. A Global Morphology Catalog in A2744 Based on UNCOVER/MegaScience

Authors: Yunchong Zhang, Tim B. Miller, Sedona H. Price, Katherine A. Suess, Rachel Bezanson, David J. Setton, Joel Leja, Katherine E. Whitaker, Jenny E. Greene, Robert Feldmann, Seiji Fujimoto, Themiya Nanayakkara, Gabriel Brammer, Sam E. Cutler, Pratika Dayal, Anna de Graaff, Yoshinobu Fudamoto, Lukas J. Furtak, Andy D. Goulding, Gourav Khullar, Ivo Labbe, Brian Lorenz, Danilo Marchesini, Abby Mintz, Lamiya A. Mowla, Adam Muzzin, Erica J. Nelson, Richard Pan, Natalia Porraz Barrera, Edward N. Taylor, Arjen van der Wel, Bingjie Wang, 冰洁王, John R. Weaver, Christina C. Williams

Yunchong Zhang et al 2026 The Astrophysical Journal Supplement Series 285 .

Provider: AAS Journals

Caption: Figure 9.

The left panel shows the redshift versus stellar mass for valid sources in F444W in the UNCOVER/MegaScience photometric catalog (use_phot = 1; gray) and all sources with a great or robust fitin F444W from this work (use_fit = 1 or 2; red). The right panel shows the net completeness of our fits in F444W, binned by redshift and stellar mass. We define completeness as the fraction of use_fit = 1 or 2 sources among use_phot = 1 sources. We omit any bins containing fewer than 10 use_phot = 1 sources. Overall, we achieve >80% net completeness at M_* > 10⁸M_⊙ and z < 2; M_* > 10^8.5M_⊙ and 2 < z < 4; M_* > 10⁹M_⊙ and 4 < z.

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