Multi-band SED of the persistent emission of SGR 1935+2154. Black lines show the best fit emission model in the X-ray and soft gamma-ray bands (Borghese et al. 2022). In the VHE band, our 95% confidence level ULs confirm the non-detection obtained by H.E.S.S. Collaboration (2021). The tera-electronvolt ULs are about the same order of magnitude as the X-ray emission and confirm previous studies, which suggest that the power-law component observed above > 10 keV must have a break at MeV energies.