The plots comparing the difference in the SFR (log(ΔSFR) = logSFR_{post − merger} - logSFR_{non − interacting}) of the post-merger concerning their non-interacting control dwarfs. Left panel: This figure shows the histogram distribution of SFR offset for the entire galaxy, central, and outer regions for those dwarfs spanning a stellar mass range of 10⁸ − 10⁹M_⊙. Right panel: This figure shows the histogram distribution of SFR offset for the visually identified dwarf galaxy sample, central and outer regions within a stellar mass range of 10⁹ − 10^9.6M_⊙.