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Fig. 11.

image

Left: stellar masses estimated from: IRAC1 measurement in Perley et al. (2016, red), this work with either a delayed or delayed  +  burst SFH (green), CIGALE using same configuration as in Table 2 but with a continuous SFH with a main stellar population age between 1 and 3.5 Gyr (blue). Right: SFR estimated from: Hα measurement from Krühler et al. (2015) and Vergani et al. (2017, red) this work using either a delayed or delayed  +  burst SFH (green), CIGALE using same configuration as in Table 2 but with a continuous SFH with a main stellar population age between 1 and 3.5 Gyr (blue).

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