Spectral energy distribution of gamma-ray emission from SS 433. Colored markers indicate flux measurements obtained with H.E.S.S. and HAWC. More recent data obtained by LHAASO are shown with black markers. The upper limits imposed by Fermi-LAT on the GeV emission from the eastern (E) and western (W) jets are overplotted with colored downward-pointing arrows. The predicted (hadronic) gamma-ray spectrum from the bubble is overplotted for the two scenarios presented in Fig. 1. The shaded region shows the expected range of gamma-ray emission when varying the terminal wind speed by a factor of two.