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Fig. 17.

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Fraction of early-type galaxies as a function of Δlog SFR. Each panel shows a different redshift bin – 0 < z < 1, 1 < z < 3, 3 < z < 6 – from left to right. The red dashed, green dotted and solid blue lines show galaxies with stellar masses of 10.5 < log M*/M < 11.5, 9.5 < log M*/M < 10.5, 9.5 < log M*/M < 10.5 respectively. The morphology-quenching relation seems to be in place for massive galaxies at z > 3.

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