OIR vs. X-ray correlation for low-mass black-hole X-ray binaries in low, hard and high, soft states, with all data points taken from Russell et al. (2006). The central line represents the best power law fit for low, hard data points: . We added the J,H, and K_s data points of H 1743-322 reported in this paper (observations # 1, 4, 6, and 8 corresponding to HSS and observation #10 corresponding to LHS, respectively), computed at the distance of 8.5 kpc. The dashed line corresponds to the different positions of Obs. #10 (triangle) in LHS, computed for distances between 2 and 13 kpc. We see that while HSS data points of H 1743-322 are consistent with HSS data points of other sources, LHS data points of H 1743-322 are clearly located below the LHS data points of other sources, precisely between LHS and HSS data points of other sources.