Specific SFR (SFR normalized to the total mass of the galaxy) of FRB 20201124A (magenta star), other repeating FRBs (light blue circles), non-repeating FRBs from Heintz et al. (2020) (dark blue circles), and our own Galaxy (light purple pentagon; Licquia & Newman 2015). For FRB 20201124A we display the specific SFR derived from radio observations (Appendix A) with a magenta star, and a dashed line connects this value to the magenta circle representing the specific SFR derived from optical spectroscopy (Appendix E and Fig. F.2). We also display the populations of other astrophysical transients for reference by including the low redshift (z < 0.3) populations of long gamma-ray bursts (LGRBs; small blue diamonds), core-collapse supernovae (CCSNe; small gray circles), and superluminous supernovae (SLSNe; small gray squares) from Taggart & Perley (2021). These values are compared to the low redshift (z < 0.05) star-forming main sequence from Saintonge et al. (2016), displayed by a solid line. Our object is located well above the SF main sequence, above which galaxies have enhanced SF efficiencies.