Fig. 12.
SFE normalised to the expected SFE assuming the relation valid for MS galaxies from Eq. (5) as a function of offset from the MS (starburstiness) for ALMA IDs 3 and 8 (filled stars), and for sources from the literature with 1 < z < 3 (filled squares: cluster galaxies, filled triangles: proto-cluster galaxies). The horizontal and vertical solid lines represent, respectively, SFEs and starburstiness values of MS galaxies, and the grey region indicates SFRs consistent with the MS within a factor of 3.
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