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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 B1.

The distribution of galaxy mass-weighted age, AV and ﹩\mathrm{log}(Z/{Z}_{\odot })﹩ with respect to the size of the semimajor axis of our annuli photometry for our “fiducial” model, demonstrating the effect of the strong metallicity Gaussian prior set by the values from C24, and the strong dust prior set via modeling including MIRI photometry. Colors, lines, and symbols are identical to Figure 3.

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