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Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-early Star Formation Tensions

  • Authors: Sam E. Cutler, Luke Robbins, Danilo Marchesini, Katherine A. Suess, Adam Muzzin, Gabriel Brammer, Yoshihisa Asada, Nicholas S. Martis, Stacey Alberts, Jacqueline Antwi-Danso, Aidan P. Cloonan, Ivo Labbé, Tim B. Miller, Ikki Mitsuhashi, Alexandra Pope, Anna Sajina, Ghassan T. E. Sarrouh, Monu Sharma, Mauro Stefanon, Edgar P. Vidal, Chris J. Willott, Rachel Bezanson, Maruša Bradač, Olivia R. Cooper, Robert Feldmann, Ben Forrest, Karl Glazebrook, Jenny E. Greene, Valentina La Torre, Jamie Lin, Michael V. Maseda, Ian McConachie, Themiya Nanayakkara, Gaël Noirot, Richard Pan, Kesha A. Patel, Veronica Pratt, Marcin Sawicki, David J. Setton, John R. Weaver, Arjen van der Wel, Katherine E. Whitaker, Yunchong Zhang, Kumail Zaidi

Sam E. Cutler et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure D1.

Posterior SEDs for each of our ultramassive quiescent galaxies using our PROSPECTOR modeling of the super and MIRI combined photometry. Median model spectra and photometry, as well as their respective 1σ uncertainties, are shown. The observed data are shown in red. Inset are the posterior distributions of AV for each object. The median of each distribution is shown as the vertical solid black line, and the upper and lower 1σ uncertainties are shown as dotted black vertical lines.

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