Left panel: Detected shocks cells for the pulsar radio state (b0) (also see Fig. 5), with the color scale representing the intensity of the rest-frame synchrotron emission normalized to its maximum value. Arrows indicate the lines of sight corresponding to the vectical lines with the same colors on the right panel. Right panel: Associated X-ray light curve. The orange and blue dashed lines correspond respectively to the star and pulsar inferior conjunctions (at 0.25 and 0.75 of the orbital phase). The vertical magenta and green dashed lines correspond to the angles with the maximum intensity received from the system.