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Fig. 7.

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UVJ colors of high-z QGs (z > 2.5) adapted from D’Eugenio et al. (2020). The post-star burst region is demarcated with the red box as specified in Belli et al. (2019). The marker sizes are proportional to the stellar mass. The red and blue stars are the dust uncorrected and corrected measurements of the quiescent stellar disks in the three star-forming galaxies within our sample. The final star in orange marks the location of Galaxy-D, a quiescent galaxy photometrically confirmed to be part of RO-1001 (Kalita et al. 2021a).

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