Fig. 3.

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Inferred star formation rate against stellar mass for the galaxies studied in this work. Results from BAGPIPES are shown in black circles, whereas those from CIGALE are shown in grey squares. The SFR upper limit (F200D_JWIDF_M03 fitted with CIGALE) is shown at the 2σ level. The coloured lines show the galaxy main sequence at z = 2, 3, 4 from Schreiber et al. (2015).
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