in the extraction region and that this makes our analysis consistent with that of @itmismma02, we chose to include it in our final fits. We find a photon index for the power-law component of $1.71_{-0.17}^{+0.13}$, and its normalization corresponds to a 1 keV flux density of $39.9_{-4.1}^{+4.6}$ nJy. Parameters for the best-fitting models are given in Table \[spectroanalysis\]. For completeness, we also attempted to model the lobes with an [*apec*]{} model alone, but this gave a significantly poorer fit ($\chi^2$/dof of 1650/1051) so we do not consider this model further. The temperature we find for the lobes is consistent within the errors with the temperature we determine for region 1.

### Regions outside the lobes {#outerregions}

For region 1, we adopted the same approach as described above for the lobes: the spectrum we extracted was for the whole region inside 160 arcsec and we then fixed the parameters of our best-fitting model for the AGN and lobes in the fit. The spectrum for the AGN, lobes and the environment is shown in Figure \[LS\]. The spectrum for the outer region (region 4) is shown in Figure \[ORspectra\]. The model for the extended emission in this region was an [*apec*]{} model 