Computed non-thermal model including a thermal Bremsstrahlung absorbed component for the IRAS 16547−4247 north lobe. The black solid line represents the total thermal and non-thermal emission from the two lobes of the system. X-ray and radio data-points are also plotted, together with the Fermi-LAT three-year (inner Galaxy) 5σ sensitivity curve and the SED for 1% of the Crab Nebula flux, the typical sensitivity of the current Cherenkov telescopes for ~50 h of observation.