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Fig. 14.

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NUVrJ diagrams showing the separation of active and passive galaxies in 0.5<z<1 in COSMOS2020. The dashed line is from Ilbert et al. (2013). Top left: Fraction of passive galaxies (colours) selected as those with a LePHARE estimate of log(sSFR/yr−1)<−11. Top right: Same fraction from sSFRs estimated by our SBI method using all filters. Bottom left: Distribution of dust, as estimated by LePHARE. Bottom right: Same fraction from sSFRs estimated by our SBI method, but without the H Band. The SFH inferred by SBI without the H band on the right side of the panel corresponds to more passive galaxies than estimated with an SED fitting, which identifies these galaxies as active, but dusty.

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