Fig. 7.
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re vs. stellar mass for the galaxies in our sample (squares). We also show quiescent galaxies at z ∼ 0.7 from LEGA-C (circles, van Houdt et al. 2021), three lensed quiescent galaxies at z ∼ 2 (diamonds, Newman et al. 2018), and galaxies at z ∼ 0 from the SAMI (van Houdt et al. 2021), MASSIVE (Veale et al. 2017), and ATLAS3D (Emsellem et al. 2011) surveys as red stars. The LEGA-C and SUSPENSE points are coloured by Vre, and the galaxies for which we could only obtain lower limits for Vre are shown in grey. We show the linear fit to quiescent galaxies at z ∼ 1.75 from the 3D-HST+CANDELS survey (van der Wel et al. 2014) in grey, with the dashed lines indicating the 1σ scatter.
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