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Fig. 5.

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Vre/σ0 as a function of stellar mass for the 15 distant quiescent galaxies in our sample (squares). The grey squares indicate galaxies for which we can only obtain lower limits to Vre/σ0. We also show quiescent galaxies at z ∼ 0.8 from LEGA-C (circles, van Houdt et al. 2021) and three lensed quiescent galaxies at z ∼ 2 (diamonds, Newman et al. 2018). The dashed line indicates a ratio of 1, corresponding to the definition of rotational support. The symbols are coloured by Vre.

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