Negative age gradients and flat [Fe/H] gradients in high-redshift quiescent galaxies from NIRSpec-MSA spectroscopy suggest cores formed and quenched earlier than outskirts.
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Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.
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Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE
Negative age gradients and flat [Fe/H] gradients in high-redshift quiescent galaxies from NIRSpec-MSA spectroscopy suggest cores formed and quenched earlier than outskirts.
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Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.