(a) Fermi-LAT GeV spectrum of the LHAASO/H.E.S.S. source counterpart (red points) obtained using the Y. Su et al. (2017) N_p map (with a radius of ﹩0\mathop{.}\limits^{^\circ }87﹩) as a template. The best-fit spectral models for LHAASO J1912+1014u in Z. Cao et al. (2024) are also plotted. (b) The TS map in ≥12.8 GeV obtained using the Y. Su et al. (2017) N_p map. (c) and (d) are the same as panels (a) and (b), respectively, but obtained using LHAASO KM2A Gaussian.