  We address the possibility of realizing successful leptogenesis from dark
matter annihilations in the scotogenic model of neutrino masses to explain the
same order of magnitude abundance of dark matter and baryons in the present
Universe. After showing that the minimal model in this category cannot satisfy
all these requirements, we study a minimal extension of this model and find
that the scale of leptogenesis can be as low as 5 TeV, lower than the one in
vanilla leptogenesis scenario in scotogenic model along with the additional
advantage of explaining the baryon-dark matter coincidence. Due to such low
scale, the model remains predictive at dark matter direct detection and rare
decay experiments looking for charged lepton flavor violating processes.
