Specific SFR vs. stellar mass relation for the host of GRB 190114C and other long GRB hosts. The specific SFR was obtained by weighting it with the stellar mass. References to the comparison samples are the same as in Fig. 7, we also add a sample of star-forming galaxies from the VUDS survey (Calabrò et al. 2017), but leave out the MASSIVE sample. SFRs for the comparison samples were largely derived by SED fitting, except for the KMOS3D sample. The grey lines are fits with a broken power law and a cut-off mass of log M = 10.2 M_⊙ at different redshifts derived by Whitaker et al. (2014). Error bars for the comparison samples are omitted for clarity.