Comparison of the observed quiescent SMF with semianalytical models and hydrodynamical simulations. These include SHARK (Lagos et al. 2018, 2024) run with two alternative runs with slow and fast ram-pressure stripping, GALFORM (Lacey et al. 2016), GAEA (De Lucia et al. 2024), SIMBA (Davé et al. 2019), EAGLE (Schaye et al. 2015; Crain et al. 2015), AND TNG100 (Springel et al. 2018; Pillepich et al. 2018). They were computed using a UVJ color selection and include uncertainties by convolving the stellar masses with a Gaussian kernel of 0.3 dex.