Stellar population gradients at cosmic noon as a constraint to the evolution of passive galaxies

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Fig. 4.

F160W S/N of the inner and outer zones. The filled symbols indicate the galaxies described in the text. S/Ns are given for a single imaging pixel (0.06 × 0.06 arcsec²), but they were calculated as the average S/N over larger areas (∼10 for the inner zone, and ∼400 for the outer zone).

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