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Searching within Galaxies for the Earliest Signs of Quenching With Spatially Resolved Star Formation Histories in UVCANDELS Galaxies at z < 0.3

  • Authors: Charlotte Olsen, Eric Gawiser, Charlotte Welker, Harry Teplitz, Kartheik Iyer, Xin Wang, Marc Rafelski, Rogier A. Windhorst, Anton Koekemoer, Anahita Alavi, Ben Sunnquist, Norman Grogin, Yicheng Guo, Christopher J. Conselice, L. Y. Aaron Yung, Kalina Nedkova, Bahram Mobasher, Ray A. Lucas, Vihang Mehta, Y. Sophia Dai, Jonathan P. Gardner

Charlotte Olsen et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 22.

The projected radial profile of UVCANDELS ID 10335 shows similar shapes for all properties: log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩, log ΣSFR, AV, and tx are highest at the galactic center and decline out to 20 kpc. Around 22 kpc, all properties rise again before dropping sharply in the outskirts. This increase corresponds to the bright star-forming knot in the postage stamps, and the outer depression aligns with the tidal feature beyond the disk.

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