and because of this the data quality was poor and we were not able to constrain the temperature.

Results
-------

In this section we describe the results of spectral fitting to each of the regions described above.

### The AGN

The model we used was a model that has been successfully fitted for other NLRGs, consisting of a Galactic absorbed power law together with an intrinsically absorbed power law and an iron K$\alpha$ line, which gives a very good fit to the data. Parameters of the best-fitting model are given in Table \[agnspec\]. We use a fixed photon index of 2.00 for the soft power-law component following [@hec06], since the photon index is poorly determined.

  Model              Parameter                                              Value
  ------------------ ------------------------------------------------------ -------------------------------------
  apec               kT(keV)                                                $0.055_{-0.003}^{+0.012}$
                     Normalization ($10^{14}$ cm$^{-5}$)                    $3.05\pm1.95\times10^{-4}$
                     kT(keV)                                                $0.31\pm0.01$
                     Normalization ($10^{14}$ cm$^{-5}$)                    $2.26_{-0.37}^{+0.20}\times10^{-5}$
  zwabs              nH ($10^{22}$cm$^{-2}$)                                0.1130
  powerlaw           Photon Index                                           1.41
                     Normalization (photons keV$^{-1}$ cm$^{-2}$s$^{-1}$)   $8.08_{-0.19}^{+0.37}\times10^{-5}$
  [$\chi^2$/dof]{}   789/468                                                

-2.0cm

  Model                                                 Parameter                                              Value
  ----------------------------------------------------- ------------------------------------------------------ -------------------------------------
  wabs                                                  nH ($10^{22}$cm$^{-2}$)                                0.1130 (fixed)
  powerlaw                                              Photon Index                                           2.00 (fixed)
                                                        Normalization (photons keV$^{-1}$ cm$^{-2}$s$^{-1}$)   $1.03_{-0.26}^{+0.03}\times10^{-4}$
  zwabs                                                 nH ($10^{22}$cm$^{-2}$)                                $43.59_{-4.37}^{+5.27}$
                                                        Redshift                                               0.0811
  \[2pt\] powerlaw                                      Photon index                                           $1.26_{-0.27}^{+0.32}$
                                                        Normalization (photons keV$^{-1}$ cm$^{-2}$s$^{-1}$)   $6.42_{-2.19}^{+9.33}\times10^{-4}$
  Gaussian                                              E(keV)                                                 $6.42\pm0.02$
                                                        $\sigma$                                               $0.08\pm0.03$
                                                        Normalization (photons cm$^{-2}$ s$^{-1}$)             $1.76_{-0.32}^{+0.35}\times10^{-5}$
  Unabsorbed 0.5 - 