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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 7.

log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlation fit lines for all galaxies are shown on the left at 1 Gyr lookback time and on the right at the time of observation. The gray shading shows the rolling 1σ confidence interval for all regions of all galaxies. At 1 Gyr lookback time, all galaxies lie on the same SFR–M∗ correlation, but the differing slopes and normalizations at the time of observation suggest that galaxies have since begun quenching in different ways.

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