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We show that the jet power $P_j$ and geometrically corrected $\gamma$-rayluminosity $L_\gamma$ for the X-ray binaries (XRBs) Cygnus X-1, Cygnus X-3, andV404 Cygni, and $\gamma$-ray upper limits for GRS 1915+105 and GX339-4, followthe universal scaling for the energetics of relativistic jets from black hole(BH) systems found by Nemmen et al. (2012) for blazars and GRBs. The observedpeak $\gamma$-ray luminosity for XRBs is geometrically corrected; and theminimum jet power is estimated from the peak flux density of radio flares andthe flare rise time. The $L_\gamma-P_j$ correlation holds across $\sim 17$orders of magnitude. The correlation suggests a jet origin for the high energyemission from X-ray binaries, and indicates a common mechanism or efficiencyfor the high energy emission 0.1-100 GeV from all relativistic BH systems.

Extending the "Energetic Scaling of Relativistic Jets From Black Hole Systems" to Include $\gamma$-ray-loud X-ray Binaries