(a) Fermi-LAT GeV spectrum of the LHAASO/H.E.S.S. source counterpart (red points) obtained using the H. Sano et al. (2018) N_p map (with a radius of ﹩0\mathop{.}\limits^{^\circ }87﹩) as a template. The best-fit spectral models for LHAASO J1912+1014u, as reported by Z. Cao et al. (2024), are also plotted. (b) The TS map in ≥12.8 GeV obtained using the H. Sano et al. (2018) N_p map.