Figure 3: Left panel: The upper limit on the annihilation cross section derived in this work for the b ¯ b channel (blue solid line), compared to other results involving antiproton analyses of [ 24 ] . The red solid line corresponds to the Giesen et al. upper bound [ 11 ] . The limits set by Cuoco et al. [ 14 ] (orange dot-dashed curve) and Cui et al. [ 15 ] (green dashed line) are also featured. Right panel: The upper limit on the annihilation cross section derived in this work for the b ¯ b channel (blue solid line), compared to other probes. The red contour is the 95% CL contour of the fit to the Galactic Center excess reported by Calore et al. in [ 78 ] for the same annihilation channel. We also display bounds from different samples dwarf spheroidal galaxies (dSph) derived with a new data-driven method by Alvarez et al. in [ 79 ] (green solid line), with traditional template-fitting strategies by Albert et al. in [ 80 ] (green dashed line), and by combining Fermi-LAT and ground-based telescopes data by Abdalla et al. in [ 81 ] (Glory Duck project, green dot-dashed line). The yellow band are ra- dio constraints derived from the EMU survey [ 82 ] . The thermal relic cross section reported in dotted black lines is the one computed in [ 83 ] . See text for