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Fig. 4.


Location of our ALMA detected galaxies in the SFR–M plane. Galaxies with Herschel counterparts are color-coded as a function of the fgas. The other galaxies are represented by gray dots. We have rescaled all of the SFRs by multiplying by SFRMS(z)/SFRMS(z = 2.7), in order to maintain their relative positions with respect to the main sequence. We indicated the MS using Eq. (9) from Schreiber et al. (2015), with a dispersion of 0.3 dex (solid and dashed lines respectively).

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