Image Details
Caption: Figure 20.
Radial profiles for 08062 in log ΣSFR, log sSFR, AV, and tx mass formation times show similar log ΣSFR shapes at both time steps, indicating little radial migration. Notably, the observed log sSFR is lower than that 1 Gyr ago in the outskirts, providing early evidence for outside-in quenching.
© 2026. The Author(s). Published by the American Astronomical Society.