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Fig. 2.

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Normalised distribution of CIGALE-inferred Bayesian parameters of the parent sample of 4583 QGs and the 460 QGs in our A3COSMOS/A3GOODSS sample: SFR fraction (rSFR), stellar mass (M*), time since quenching (tq), and (ΔMS) before quenching and at the time of observation. We note that, due to the re-estimation of M* with CIGALE, a small number of galaxies fall slightly below the initial selection threshold of log(M*/M) = 10.8.

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