Accelerated calibration of semi-analytic galaxy formation models
A fast likelihood framework for calibrating semi-analytic galaxy formation models using stellar-to-halo mass relation constraints, demonstrated with Galacticus.
A fast likelihood framework for calibrating semi-analytic galaxy formation models using stellar-to-halo mass relation constraints, demonstrated with Galacticus.
Reanalysis of the strong lens SDSS J0946+1006 showing that its apparent high-density subhalo can be naturally explained if the perturber hosts a faint satellite galaxy.