Adaptation of Fig. 10 of Harding et al. (2021) showing the two models derived in the paper for the SC emission of Geminga, together with the LST-1 P2 SED obtained in this work (same as Fig. 4). The Fermi-LAT and MAGIC points from the analysis presented in this work and MAGIC Collaboration (2020), respectively, are also reported for comparison. Note that the Fermi-LAT points represent the phase-averaged flux, i.e. they take into account the emission from both P1 and P2.