Fig. 1.
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Upper panel: U–V and V–J colour selection colour-coded by redshift for the massive quiescent galaxies in our full sample. The black line corresponds to the Schreiber et al. (2015) quenching criterion with the grey line addition of the Belli et al. (2019) fast quenching criterion. The dotted red line corresponds to the selection criteria from Baker et al. (2025a) which we use as our initial selection criteria in this work.
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