Table 3: Best fit parameters when a LAOR component is added to the BMS, with the emissivity law $\beta $ fixed to -2. The values for $\beta $ and $\chi ^{2}_{\beta }$ refers to the fit where the $r_{\rm out}$ parameter is fixed to 400 $r{\rm _g}$ (see text for details).
Object ${N}_{\rm H}$ $\Gamma$ R ${E}_{\rm c}$ EW $r{\rm _{out}}$ $\chi^2$/d.o.f. $\beta $ $\chi ^{2}_{\beta }$/d.o.f.
  $\times10^{22}$ cm-2     (keV) (eV) ($r{\rm _g}$)      
ESO198-G024 - $\rm 1.95^{+0.12}_{-0.10}$ $\rm 1.10^{+0.98}_{-0.56}$ >260 $\rm 210^{+116}_{-124}$ $\rm 4.6^{+2.3}_{-0.7}$ 96/124 $\rm 4.5^{+1.8}_{-1.1}$ 97/124
MCG-02-58-022 - $\rm 1.75^{+0.08}_{-0.07}$ $\rm0.40^{+0.37}_{-0.26}$ $\rm 230^{+520}_{-110}$ $\rm 90^{+92}_{-72}$ >22 123/132 <3 123/132
NGC 7213 - $\rm 1.68^{+0.04}_{-0.06}$ <0.55 $\rm 100^{+290}_{-50}$ $\rm 111^{+39}_{-66}$ $3.1\pm0.2$ 161/178 $\rm 6.5^{+1.4}_{-0.9}$ 163/178
NGC 5548 - $\rm 1.66^{+0.03}_{-0.05}$ $\rm0.48^{+0.21}_{-0.14}$ $\rm 160^{+90}_{-40}$ $\rm 66^{+23}_{-31}$ $\rm 2.7^{+0.2}_{-0.1}$ 194/193 $\rm 6.8^{+0.9}_{-1.1}$ 188/193
MKN 841 - $\rm 1.86^{+0.14}_{-0.12}$ $\rm 1.49^{+0.75}_{-0.90}$ $\rm 80^{+290}_{-40}$ $\rm 158^{+77}_{-83}$ $\rm 2.3^{+0.2}_{-0.1}$ 97/135 $7.8\pm1.2$ 99/135
IC 4329A $0.27\pm0.01$ $1.84\pm0.01$ $0.50\pm0.06$ $170\pm20$ $\rm 298^{+102}_{-87}$ $5.5\pm0.1$ 248/208 $\rm 3.6^{+1.5}_{-0.2}$ 265/208
NGC 3516 $\rm 2.2^{+0.4}_{-0.3}\times 10^{-2}$ $\rm 1.49^{+0.02}_{-0.04}$ $\rm0.53^{+0.17}_{-0.14}$ $\rm 100^{+30}_{-20}$ $\rm 209^{+43}_{-49}$ $\rm 4.8^{+0.8}_{-0.6}$ 269/257 $\rm 4.8^{+0.9}_{-0.4}$ 260/257
NGC 5506 $\rm 2.91^{+0.04}_{-0.05}$ $\rm 1.83^{+0.08}_{-0.04}$ $\rm 1.04^{+0.20}_{-0.16}$ $110\pm20$ $\rm 124^{+56}_{-49}$ $\rm 2.7^{+0.3}_{-0.1}$ 286/256 $\rm 6.2^{+1.5}_{-1.3}$ 290/256


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