Table 2: Best fit parameters for the BMS. The second-last column refers to the addition of a DISKLINE component to the model (see text for details). Note that the BMS includes, in some cases, additional features when required by the data: see the analysis of individual sources for details.
Object ${N}_{\rm H}$ $\Gamma$ R ${E}_{\rm c}$ $E_{\rm Fe}$ EW $\sigma$ disk EW $\chi^2$/d.o.f.
  $\times10^{22}$ cm-2     (keV) (keV) (eV) (eV) (eV)  
ESO198-G024 - $\rm 1.91^{+0.11}_{-0.07}$ $\rm0.86^{+0.41}_{-0.64}$ >260 $6.38\pm0.06$ $\rm 57^{+30}_{-29}$ <160 <150 103/123
MCG-02-58-022 - $\rm 1.72^{+0.08}_{-0.06}$ $\rm0.41^{+0.27}_{-0.30}$ $\rm 150^{+300}_{-50}$ $\rm 6.29^{+0.26}_{-0.06}$ $\rm 45^{+85}_{-24}$ <340 <140 127/131
NGC 7213 - $\rm 1.68^{+0.03}_{-0.02}$ <0.19 $\rm 90^{+50}_{-20}$ $\rm 6.39^{+0.01}_{-0.02}$ $\rm 82^{+16}_{-14}$ <60 <20 174/177
NGC 5548 - $1.68\pm0.03$ $\rm0.45^{+0.20}_{-0.16}$ $\rm 190^{+140}_{-60}$ $\rm 6.38^{+0.02}_{-0.03}$ $\rm 58^{+15}_{-14}$ $\rm 63^{+45}_{-58}$ <40 206/192
MKN 841 - $\rm 1.97^{+0.11}_{-0.10}$ $\rm 1.31^{+1.21}_{-0.70}$ >100 $6.35\pm0.05$ $\rm 96^{+44}_{-35}$ $\rm 88^{+60}_{-53}$ <40 107/134
IC 4329A $0.26\pm0.01$ $1.78\pm0.01$ $\rm0.30^{+0.05}_{-0.06}$ $130\pm10$ $6.42\pm0.05$ $\rm 127^{+32}_{-37}$ $\rm 108^{+53}_{-37}$ <50 263/207
NGC 3516 $\rm 4.3^{+0.2}_{-0.1}\times 10^{-2}$ $1.56\pm0.01$ $\rm0.50^{+0.08}_{-0.07}$ $120\pm20$ $\rm 6.40^{+0.01}_{-0.02}$ $\rm 106^{+15}_{-10}$ $\rm 40^{+20}_{-23}$ <20 296/256
NGC 5506 $\rm 3.02^{+0.04}_{-0.05}$ $\rm 1.88^{+0.05}_{-0.02}$ $\rm 1.10^{+0.19}_{-0.14}$ $\rm 140^{+40}_{-30}$ $6.41\pm0.02$ $100\pm19$ $\rm 59^{+32}_{-33}$ <40 297/255


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