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A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn

  • Authors: Elizabeth J. McGrath, Steven L. Finkelstein, Guillermo Barro, Viraj Pandya, Henry C. Ferguson, Jeyhan S. Kartaltepe, Dale D. Kocevski, Ricardo O. Amorín, Bren E. Backhaus, Fernando Buitrago, Antonello Calabrò, Yingjie Cheng, Luca Costantin, Isa G. Cox, Kelcey Davis, Giovanni Gandolfi, Yuchen Guo, Nimish P. Hathi, Michaela Hirschmann, Benne W. Holwerda, Marc Huertas-Company, Anton M. Koekemoer, Ray A. Lucas, Bahram Mobasher, Fabio Pacucci, Casey Papovich, Pablo G. Pérez-González, Jonathan R. Trump, L. Y. Aaron Yung, Pablo Arrabal Haro, Micaela B. Bagley, Mark Dickinson, Adriano Fontana, Andrea Grazian, Norman A. Grogin, Lisa J. Kewley, Allison Kirkpatrick, Jennifer M. Lotz, Laura Pentericci, Nor Pirzkal, Swara Ravindranath, Rachel S. Somerville, Stephen M. Wilkins, Guang Yang, Lise-Marie Seillé, Xin Wang

Elizabeth J. McGrath et al 2026 The Astrophysical Journal Letters 999 .

  • Provider: AAS Journals

Caption: Figure 9.

Color gradient, as defined in Equation (3), is shown as a function of redshift and mass. Individual galaxy points are color coded according to their Sérsic index with n < 2.5 shown as blue, and n > 2.5 shown as red. The mean relation, along with the 16th−84th percentile range are shown for n < 2.5 and n > 2.5 galaxies as the blue and red lines and shaded regions, respectively. We find that there is no evidence for variation in color gradients as a function of redshift for either low- or high-Sérsic-index galaxies, and color gradients are slightly negative on average. We also find evidence for larger color gradients among the most massive galaxies, a trend that is most evident for low-n sources.

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