Fig. 5.
Likelihood of the photometric data for Hyde as a function of sSFR = SFR/M*. The likelihood is shown without any constrain on the dust luminosity (gray), using the total infrared luminosity LIR (orange), or using the birthcloud infrared luminosity LIR, BC (red). The horizontal red lines show the 68% (thick) and 90% (thin) confidence intervals. The vertical lines indicate the locus of the galaxy main-sequence and its scatter from Schreiber et al. (2017).
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