EAGLE and TNG100 simulations largely reproduce the spectral covariance of SDSS galaxies, but AGN feedback differences, traced to black hole seeding, cause subtle mismatches in quiescent and AGN populations.
G., Dalla Vecchia C., Pillepich A.
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Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
EAGLE and TNG100 simulations largely reproduce the spectral covariance of SDSS galaxies, but AGN feedback differences, traced to black hole seeding, cause subtle mismatches in quiescent and AGN populations.