Table 4: Best fit parameters when the BMS is modified by replacing the narrow iron line with a DISKLINE (see text for details).
Object ${N}_{\rm H}$ $\Gamma$ R ${E}_{\rm c}$ $E_{\rm Fe}$ EW $r{\rm _{out}}$ $\chi^2$/d.o.f.
  $\times10^{22}$ cm-2     (keV) (keV) (eV) ($r{\rm _g}$)  
ESO198-G024 - $\rm 1.91^{+0.04}_{-0.03}$ $\rm0.86^{+0.83}_{-0.30}$ >350 $\rm 6.4^{+0.8}_{-0.5}$ $\rm 71^{+34}_{-39}$ >3000 106/123
MCG-02-58-022 - $\rm 1.74^{+0.08}_{-0.06}$ $\rm0.38^{+0.38}_{-0.26}$ $\rm 220^{+780}_{-100}$ $\rm 6.39^{+0.09}_{-0.13}$ $\rm 131^{+63}_{-60}$ >170 122/131
NGC 7213 - $\rm 1.68^{+0.05}_{-0.04}$ <0.32 $\rm 100^{+300}_{-50}$ $\rm 6.39^{+0.02}_{-0.01}$ $\rm 100^{+19}_{-16}$ > $4\times10^5$ 178/177
NGC 5548 - $\rm 1.68^{+0.03}_{-0.02}$ $\rm0.45^{+0.19}_{-0.16}$ $\rm 200^{+80}_{-70}$ $\rm 6.37^{+0.03}_{-0.02}$ $\rm 67^{+13}_{-15}$ >20 000 205/192
MKN 841 - $\rm 1.96^{+0.04}_{-0.08}$ $\rm 1.25^{+0.31}_{-0.69}$ $\rm 170^{+370}_{-70}$ $6.35\pm0.06$ $\rm 108^{+40}_{-38}$ >3 500 110/134
IC 4329A $0.26\pm0.01$ $1.78\pm0.01$ $\rm0.30^{+0.04}_{-0.06}$ $130\pm15$ $\rm 6.38^{+0.09}_{-0.03}$ $\rm 193^{+26}_{-84}$ >800 266/207
NGC 3516 $4.4\pm0.2\times 10^{-2}$ $1.56\pm0.01$ $0.47\pm0.07$ $120\pm20$ $\rm 6.40^{+0.01}_{-0.02}$ $131\pm16$ > $1\times10^6$ 303/256
NGC 5506 $\rm 3.02^{+0.03}_{-0.06}$ $\rm 1.88^{+0.05}_{-0.04}$ $\rm 1.09^{+0.20}_{-0.13}$ $\rm 140^{+40}_{-30}$ $\rm 6.40^{+0.03}_{-0.01}$ $\rm 117^{+20}_{-22}$ >24 000 299/255


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