Stellar metallicity-mass relations for quiescent galaxies show negligible evolution since z~0.7 while low-mass star-forming galaxies are less metal-rich at higher redshift; median ages evolve by only ~2 Gyr, requiring both passive aging and quenching of massive metal-rich star-formers to match local
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LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
Stellar metallicity-mass relations for quiescent galaxies show negligible evolution since z~0.7 while low-mass star-forming galaxies are less metal-rich at higher redshift; median ages evolve by only ~2 Gyr, requiring both passive aging and quenching of massive metal-rich star-formers to match local