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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 18.

Similar to Figure 17, we show the evolution of regions within UVCANDELS IDs 08218, 22456, and 23475. These galaxies contain more regions, and their high density obscures the variety of evolutionary tracks seen in other galaxies. UVCANDELS 08218 and 23475 in particular show many regions with log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩∼7–8.5 [M⊙ kpc−2], whose log ΣSFR typically declines steeply from a 1 Gyr lookback time.

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