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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 17.

Evolving log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlations for UVCANDELS IDs 05386 and 10335. Left: points and trend lines at the time of observation (cyan) and 1 Gyr lookback time (black). Right: more detailed evolution with additional time steps at 750, 500, and 250 Myr. These galaxies have relatively few regions, making their diverse evolutionary tracks clearly visible. All three show minor changes in slope and normalization in their correlation lines.

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