\begin{table}
\caption{\label{taba2}Best-fit parameters of the baseline models and absorption lines for the type~1 and type~2 sources.}
\begin{tabular}{l c|c c c c c c| c c c c c c c c c}
\hline\hline 
\small{Source} & \small{OBSID} & \multicolumn{6}{c}{\small{Baseline model}} & \multicolumn{9}{|c}{\small{Absorption line}} \\
%\hline
% & & & & & & & & & & & & & & & &\\
 & & $\Gamma$ & $N_{\rm H}$ & $E$ & $\sigma$ & $EW$ & $\chi^2/\nu$ & $E$ & $\sigma$ & $EW$ & $v_{\rm out}$ & $\Delta\chi^2$ & F-test & M.C. & ID & $EW$$_{{\rm MOS}}$\\ 
 & & & \scriptsize{($10^{22}$~cm$^{-2}$)} & \scriptsize{(keV)} & \scriptsize{(eV)} & \scriptsize{(eV)} & & \scriptsize{(keV)} & \scriptsize{(eV)} & \scriptsize{(eV)} & \scriptsize{($c$)} & & & & & \scriptsize{(eV)}\\
\tablefootmark{1} & \tablefootmark{2} & \tablefootmark{3} & \tablefootmark{4} & \tablefootmark{5} & \tablefootmark{6} & \tablefootmark{7}& \tablefootmark{8} & \tablefootmark{9} & \tablefootmark{10} & \tablefootmark{11} & \tablefootmark{12} & \tablefootmark{13} & \tablefootmark{14} & \tablefootmark{15} & \tablefootmark{16} & \tablefootmark{17}\\
\hline   
%& & & & & & & & & & & & & &\\%[-5pt] 
\multicolumn{17}{c}{Type~1 Sources}\\[1.2pt]
%\hline
 & & & & & & & & & & & & & & & &\\ 
NGC~4151 & 0112310101 & $1.46\pm0.04$ & $8.2\pm0.5$ & $6.398\pm0.004$ & 100 & $290\pm18$ & 1134/1064 & & & & & & & & &\\
 & 0112830501 & $1.43\pm0.04$ & $7.9\pm0.5$ & $6.397\pm0.005$ & 100 & $290\pm19$ & 1067/1021 & & & & & & & &\\
 & 0112830201 & $1.37\pm0.02$ & $7.4\pm0.1$ & $6.391\pm0.002$ & $62\pm4$ & $240\pm67$ & $1290/1309$ & & & & & & & & & \\
 & & & & $6.94\pm0.02$ & $100\pm24$ & $50\pm12$ & & & & & & & & & &\\
 & 0143500201 & $1.64\pm0.02$ & $7.2\pm0.2$ & $6.40\pm0.01$ & $79\pm10$ & $\rm 90^{+12}_{-9}$ & 1250/1317 & & & & & & & & &\\
 & 0143500301 & $1.66\pm0.02$ & $6.4\pm0.2$ & $6.40\pm0.01$ & $80\pm9$ & $80\pm10$ & 1362/1354 & & & & & & & & &\\
 & 0402660201 & $1.58\pm0.03$ & $11.0\pm0.4$ & $\rm 6.399^{+0.005}_{-0.002}$ & $79\pm8$ & $160\pm12$ & 1260/1226 & $7.74\pm0.05$ & 100 & $-32\pm7$ & $+0.105\pm0.005$ & 18 & 99.99\% & 99.7\% & Ly$\alpha$ & $-25\pm13$\\
IC4329A & 0147440101 & $1.65\pm0.01$ & & $6.40\pm0.01$ & 100 & $92\pm7$ & $1421/1388$ & $7.69\pm0.03$ & 10 & $-10\pm3$ & $+0.098\pm0.003$ & 11 & 99.5\% & 96\% & Ly$\alpha$ & $-11\pm6$\\
 & & & & $6.95\pm0.02$ & 100 & $30\pm7$ & & & & & & & & & &\\
NGC~3783 & 0112210101 & $1.77\pm0.04$ & $2.0\pm0.4$ & $6.36\pm0.01$ & 100 & $\rm 135^{+18}_{-15}$ & 1131/1076 & $6.61\pm0.02$ & 10 & $-16\pm5$ & $-0.013\pm0.004$ & 15.4 & 99.94\% & & He$\alpha$ & $-21\pm8$\\
 & & & & $7.01\pm0.02$ & 100 & $39\pm13$ & & $7.74\pm0.03$ & 10 & $-25\pm7$ & $-0.018\pm0.004$ & 12 & 99.7\% & 98.2\% & He$\beta$ & $+10\pm21$\\ 
 & 0112210201\tablefootmark{b} & $1.66\pm0.02$ & $1.9\pm0.2$ & $6.39\pm0.01$ & 100 & $\rm 150^{+10}_{-11}$ & 1290/1309 & $6.63\pm0.03$ & 10 & $-10\pm3$ & $-0.010\pm0.005$ & 13 & 99.87\% &  & He$\alpha$ & $-24\pm9$\\
 & & & & $7.01\pm0.01$ & 100 & $57\pm11$ & & & & & & & & & &\\
 & 0112210501\tablefootmark{b} & $1.74\pm0.02$ & $2.2\pm0.2$ & $6.39\pm0.01$ & 100 & $120\pm9$ & 1578/1363 & $6.67\pm0.02$ & 10 & $-17\pm2$ & $-0.004\pm0.002$ & 51 & $>$$99.99$\% & & He$\alpha$ & $-30\pm8$\\
 & & & & $7.05\pm0.02$ & 100 & $37\pm9$ & & & & & & & & & &\\
MCG+8-11-11 & 0201930201 & $1.57\pm0.01$ & & $6.42\pm0.01$ & 100 & $130\pm18$ & 981/1051 & & & & & & & & &\\
NGC~5548 & 0109960101 & $1.59\pm0.02$ & & $6.41\pm0.01$ & 10  & $72\pm18$ & 968/756 & & & & & & & & &\\
 & 0089960301 & $1.60\pm0.01$ & & $6.41\pm0.01$ & 10 & $60\pm12$ & 1221/1225 & & & & & & & & &\\
 & 0089960401 & $1.69\pm0.01$ & & $6.37\pm0.02$ & 100 & $77\pm18$ & 922/919 & & & & & & & & &\\
NGC~3516 & 0107460701 & $1.76\pm0.03$ & $8.1\pm0.4$ & $6.41\pm0.01$ & 10 & $297\pm18$ & 1194/1106 & & & & & & & & &\\
 & 0401210401 & $2.07\pm0.03$ & $3.6\pm0.4$ & $6.39\pm0.01$ & 100 & $93\pm14$ & 1285/1138 & $6.73\pm0.02$ & 10 & $-22\pm5$ & $+0.005\pm0.002$ & 27.4 & $>$$99.99$\% & & He$\alpha$ & $-30\pm7$\\
 & & & & & & & & $7.02\pm0.02$ & 10 & $-24\pm5$ & $+0.008\pm0.002$ & 21.6 & 99.99\% & & Ly$\alpha$ & $-40\pm9$\\
 & 0401210501 & $2.06\pm0.03$ & $3.8\pm0.4$ & $6.39\pm0.01$ & 100 & $125\pm15$ & 1226/1146 & $6.69\pm0.02$ & 10 & $-15\pm5$ & $-0.001\pm0.004$ & 14 & 99.6\% & & He$\alpha$ & $-33\pm7$\\
 & & & & & & & & $7.04\pm0.02$ & 10 & $-21\pm5$ & $+0.010\pm0.002$ & 20.2 & 99.99\% & & Ly$\alpha$ & $-38\pm9$\\
 & 0401210601 & $2.01\pm0.03$ & $4.9\pm0.4$ & $6.38\pm0.01$ & 100 & $\rm 133^{+16}_{-13}$ & 1170/1095 & $6.77\pm0.02$ & 10 & $-25\pm6$ & $+0.011\pm0.002$ & 26.2 & $>$$99.99$\% & & He$\alpha$ & $-29\pm7$\\
 & & & & & & & & $7.08\pm0.02$ & 10 & $-27\pm6$ & $+0.016\pm0.002$ & 17 & 99.96\% & & Ly$\alpha$ & $-31\pm9$\\
 & & & & & & & & $7.95\pm0.02$ & 10 & $-33\pm9$ & $+0.009\pm0.002$ & 24.2 & $>$$99.99$\% & $>$$99.9$\% & He$\beta$ & $-18\pm10$\\
 & & & & & & & & $8.28\pm0.03$ & 10 & $-34\pm9$ & $+0.004\pm0.004$ & 14.6 & 99.9\% & 99.5\% & Ly$\beta$ & $-20\pm15$\\
 & 0401211001 & $2.05\pm0.04$ & $3.5\pm0.4$ & $6.42\pm0.01$ & 100 & $131\pm20$ & 1067/1024 & $6.71\pm0.04$ & 10 & $-18\pm5$ & $+0.002\pm0.006$ & 10.4 & 99.3\% & & He$\alpha$ & $-31\pm7$\\
 & & & & & & & & $7.09\pm0.03$ & 10 & $-21\pm7$ & $+0.017\pm0.004$ & 12.7 & 99.8\% & & Ly$\alpha$ & $-31\pm8$\\
NGC~4593 & 0059830101 & $1.68\pm0.01$ & & $6.40\pm0.01$ & 100 & $130\pm15$ & 1212/1186 & & & & & & & & &\\
Mrk~509 & 0130720101 & $1.54\pm0.02$ & & $6.38\pm0.02$ & 100 & $84\pm23$ & 837/855 & $8.29\pm0.03$ & 10 & $-32\pm12$ & $+0.172\pm0.003$ & 9.6 & $99.3\%$ & $95\%$ & Ly$\alpha$ & $-33\pm10$\\
 & 0130720201 & $1.60\pm0.02$ & & $6.43\pm0.02$ & 100 & $60\pm19$ & 979/981 & & & & & & & & &\\
 & 0306090201 & $1.70\pm0.01$ & & $6.43\pm0.01$ & 100 & $67\pm11$ & 1059/1192 & $8.03\pm0.02$ & 10 & $-19\pm6$ & $+0.141\pm0.002$ & 15 & 99.9\% & 99.4\% & Ly$\alpha$ & $-26\pm13$\\
 & & & & $7.02\pm0.04$ & 100 & $24\pm13$ & & & & & & & & & &\\ 
 & 0306090301 & $1.72\pm0.02$ & & $6.43\pm0.02$ & 100 & $62\pm16$ & 967/1019 & & & & & & & & &\\
 & 0306090401 & $1.68\pm0.01$ & & $6.44\pm0.02$ & 100 & $58\pm12$ & 1147/1187 & $8.51\pm0.04$ & 10 & $-19\pm7$ & $+0.196\pm0.003$ & 10 & 99.5\% & 95.3\% & Ly$\alpha$ & $-11\pm7$\\
 & & & & $6.85\pm0.08$ & 100 & $22\pm12$ & & & & & & & & & &\\ 
MCG-6-30-15 & 0111570101 & $2.09\pm0.04$ & $3.4\pm0.5$ & $6.35\pm0.03$ & 100 & $\rm 78^{+24}_{-21}$ & 895/876 & & & & & & & & &\\
 & 0111570201 & $2.25\pm0.04$ & $4.1\pm0.4$ & $6.39\pm0.02$ & 100 & $67\pm15$ & 1028/1013 & & & & & & & & &\\
 & 0029740101 & $2.26\pm0.03$ & $4.4\pm0.3$ & $6.43\pm0.01$ & 100 & $78\pm13$ & 1154/1127 & & & & & & & & &\\
 & 0029740701 & $2.16\pm0.02$ & $2.8\pm0.2$ & $6.42\pm0.01$ & 100 & $65\pm10$ & 1381/1289 & & & & & & & & &\\
 & 0029740801 & $2.28\pm0.02$ & $3.8\pm0.2$ & $6.43\pm0.01$ & 100 & $\rm 79^{+16}_{-10}$ & 1338/1253 & & & & & & & & &\\
Ark~120 & 0147190101\tablefootmark{b} & $1.86\pm0.01$ & & $6.39\pm0.01$ & 100 & $90\pm15$ & 1148/1163 & $9.18\pm0.03$ & 10 & $-25\pm9$ & $+0.269\pm0.002$ & 11 & 99.6\% & 97.1\% & Ly$\alpha$ & $-10\pm24$\\
 & & & & $6.71\pm0.03$ & 100 & $43\pm13$ & & & & & & & & & &\\
 & & & & $7.02\pm0.02$ & 10 & $24\pm12$ & & & & & & & & & &\\
Mrk~110 & 0201130501 & $1.68\pm0.02$ & & $6.45\pm0.02$ & 100 & $56\pm17$ & 931/967 & & & & & & & & & \\
NGC~7469 & 0112170101 & $1.69\pm0.03$ & & $6.40\pm0.01$ & 10 & $110\pm30$ & 467/509 & & & & & & & & & \\
 & 0112170301 & $1.75\pm0.02$ & & $6.43\pm0.02$ & 100 & $96\pm29$ & 611/653 & & & & & & & & &\\
 & 0207090101 & $1.75\pm0.01$ & & $6.41\pm0.01$ & 100 & $110\pm12$ & 1145/1119 & & & & & & & & &\\
 & 0207090201 & $1.76\pm0.01$ & & $6.42\pm0.01$ & 100 & $110\pm13$ & 1131/1104 & & & & & & & & &\\
IRAS~5078+1626 & 0502090501 & $1.55\pm0.02$ & & $6.39\pm0.01$ & 100 & $120\pm18$ & 1026/978 & & & & & & & & & \\
Mrk~279 & 0302480401 & $1.74\pm0.02$ & & $6.43\pm0.01$ & 100 & $100\pm18$ & 1037/1028 & & & & & & & & & \\
 & 0302480501\tablefootmark{a} & $1.71\pm0.02$ & & $6.43\pm0.01$ & 100 & $115\pm23$ & 976/1022 & $6.69\pm0.02$ & 10 & $-19\pm9$ & $-0.001\pm0.004$ & 10.5 & 99.6\% & & He$\alpha$ & $\rm -30^{+27}_{-23}$\\
 & & & & $7.00\pm0.06$ & 10 & $29\pm16$ & & & & & & & & & &\\
 & 0302480601 & $1.70\pm0.02$ & & $6.42\pm0.01$ & 100 & $130\pm30$ & 731/753 & & & & & & & & &\\
NGC~526A & 0150940101 & $1.43\pm0.02$ & & $6.40\pm0.02$ & 100 & $90\pm19$ & 969/945 & & & & & & & & & \\
NGC~3227 & 0101040301 & $1.50\pm0.06$ & $\rm 7.3^{+1.0}_{-0.7}$ & $6.38\pm0.01$ & 100 & $\rm 220^{+61}_{-36}$ & 514/484 & & & & & & & & &\\
 & 0400270101 & $1.55\pm0.01$ & & $6.39\pm0.01$ & 100 & $112\pm11$ & 1292/1297 & & & & & & & & &\\
NGC~7213 & 0111810101 & $1.71\pm0.02$ & & $6.42\pm0.02$ & 100 & $110\pm24$ & 786/824 & & & & & & & & &\\
ESO~511-G30 & 0502090201 & $1.71\pm0.01$ & & $6.39\pm0.01$ & 100 & $100\pm15$ & 1215/1093 & & & & & & & & &\\
Mrk~79 & 0400070201 & $1.74\pm0.03$ & & $6.43\pm0.02$ & 10 & $54\pm24$ & 586/568 & $7.63\pm0.03$ & 10 & $-43\pm14$ & $+0.091\pm0.004$ & 12 & 99.5\% & 97.7\% & Ly$\alpha$ & $+6\pm32$\\
 & 0400070301 & $1.64\pm0.03$ & & $6.42\pm0.01$ & 10 & $80\pm27$ & 411/467 & & & & & & & & &\\
 & 0400070401 & $1.60\pm0.03$ & & $6.37\pm0.02$ & 100 & $115\pm36$ & 441/439 & & & & & & & & &\\
NGC~4051 & 0109141401\tablefootmark{b} & $2.04\pm0.03$ & $1.7\pm0.4$ & $6.39\pm0.01$ & 100 & $120\pm18$ & 1127/1105 & $7.10\pm0.03$ & 10 & $-19\pm6$ & $+0.018\pm0.004$ & 11.2 & 99.6\% & 97.5\% & Ly$\alpha$ & $-40\pm17$\\
 & 0157560101 & $1.77\pm0.04$ & $6.5\pm0.9$ & $6.42\pm0.01$ & 100 & $275\pm40$ & 507/436 & $8.10\pm0.05$ & 100 & $-96\pm24$ & $+0.150\pm0.005$ & 17 & 99.94\% & 99.7\% & Ly$\alpha$ & $-77\pm41$\\
 & & & & $7.08\pm0.02$ & 10 & $48\pm25$ & & & & & & & & & &\\
Mrk~766 & 0096020101 & $1.96\pm0.03$ & & $6.41\pm0.02$ & 10 & $65\pm27$ & 608/568 & & & & & & & & &\\
 & & & & $6.73\pm0.04$ & 100 & $74\pm34$ & & & & & & & & & &\\
 & 0109141301 & $2.02\pm0.02$ & & $6.39\pm0.02$ & 10 & $44\pm11$ & 1254/1089 & & & & & & & & &\\
 & & & & $6.73\pm0.04$ & 100 & $60\pm15$ & & & & & & & & & &\\
 & 0304030101 & $1.90\pm0.06$ & $6.6\pm0.8$ & $6.43\pm0.02$ & 10 & $57\pm30$ & 704/667 & & & & & & & & &\\
 & & & & $6.66\pm0.05$ & 10 & $57\pm29$ & & & & & & & & &\\
 & 0304030301 & $1.88\pm0.02$ & & $6.39\pm0.01$ & 10 & $60\pm21$ & 961/888 & $7.28\pm0.05$ & 100 & $\rm -39^{+11}_{-13}$ & $+0.044\pm0.007$  & 12 & 99.6\% & 98.6\% & Ly$\alpha$ & $-59\pm17$\\
 & & & & $6.62\pm0.04$ & 100 & $63\pm24$ & & & & & & & & & &\\
 & 0304030401 & $1.88\pm0.02$ & & $6.43\pm0.01$ & 10 & $43\pm16$ & 993/920 & & & & & & & & &\\
 & & & & $6.79\pm0.04$ & 100 & $65\pm21$ & & & & & & & & &\\
 & 0304030501 & $1.99\pm0.02$ & & $6.41\pm0.01$ & 10 & $50\pm15$ & 995/960 & $7.63\pm0.03$ & 10 & $-27\pm10$ & $+0.091\pm0.004$ & 12.2 & 99.7\% & 98.7\% & Ly$\alpha$ & $-7\pm21$\\
 & & & & $6.78\pm0.03$ & 100 & $77\pm21$ & & & & & & & & & &\\
 & 0304030601 & $1.89\pm0.02$ & & $6.35\pm0.04$ & 10 & $27\pm16$ & 1012/908 & & & & & & & & &\\
 & & & & $6.67\pm0.04$ & 100 & $52\pm23$ & & & & & & & & & &\\
 & 0304030701 & $1.70\pm0.06$ & & $6.49\pm0.04$ & 10 & $54\pm22$ & 360/329 & & & & & & & & &\\
Mrk~841 & 0205340201 & $1.80\pm0.06$ & $5.1^{+0.8}_{-1.0}$ & $6.46\pm0.02$ & 100 & $\rm 100^{+43}_{-30}$ & 491/522 & & & & & & & & &\\
 & 0205340401\tablefootmark{a} & $1.61\pm0.04$ & & $6.49\pm0.03$ & 100 & $\rm 100^{+43}_{-36}$ & 321/337 & $7.19\pm0.02$ & 10 & $-46\pm16$ & $+0.034\pm0.003$ & 12 & 99.8\% & 98.4\% & Ly$\alpha$ & $+32\pm28$\\
Mrk~704 & 0300240101 & $1.70\pm0.10$ & $5.0\pm1.2$ & $6.36\pm0.03$ & 100 & $136\pm46$ & 340/320 & & & & & & & & &\\
Fairall~9 & 0101040201 & $1.64\pm0.03$ & & $6.39\pm0.02$ & 100 & $150\pm36$ & 451/493 & & & & & & & & &\\
ESO~323-G77 & 0300240501 & $2.36\pm0.09$ & $12\pm1$ & $6.40\pm0.03$ & 100 & $\rm 115^{+49}_{-36}$ & 503/417 & $6.73\pm0.01$ & 10 & $-78\pm13$ & $+0.005\pm0.002$ & 46.2 & $>$$99.99$\% & & He$\alpha$ & $-58\pm18$\\
 & & & & & & & & $7.02\pm0.02$ & 10 & $-77\pm15$ & $+0.008\pm0.003$ & 30 & $>$$99.99$\% & & Ly$\alpha$ & $-79\pm20$\\
1H419-577 & 0148000201 & $1.21\pm0.05$ & & $6.33\pm0.05$ & 100 & $\rm 90^{+56}_{-47}$ & 197/176 & $7.23\pm0.04$ & 10 & $\rm -55^{+18}_{-21}$ & $+0.037\pm0.005$ & 10.3 & 99\% & 95.8\% & Ly$\alpha$ & $-29\pm22$ \\
 & 0148000401 & $1.55\pm0.05$ & 198/225 & & & & & & & & & & & & &\\
 & 0148000601 & $1.49\pm0.05$ & 214/213 & & & & & & & & & & & & &\\
Mrk~335 & 0101040101 & $2.00\pm0.03$ & & $6.46\pm0.08$ & 100 & $60\pm30$ & 542/543 & & & & & & & & &\\
 & 0306870101 & $1.97\pm0.01$ & & $6.41\pm0.02$ & 100 & $90\pm18$ & 1019/1018 & & & & & & & & &\\
 & & & & $6.96\pm0.02$ & 100 & $64\pm18$ & & & & & & & & & &\\
 & 0510010701 & $2.5\pm0.2$ & $13\pm2$ & $6.39\pm0.03$ & 100 & $\rm 182^{+80}_{-75}$ & 135/121 & & & & & & & & &\\
ESO~198-G024 & 0305370101 & $1.62\pm0.02$ & & $6.43\pm0.02$ & 100 & $90\pm18$ & 944/937 & & & & & & & & &\\
Mrk~290 & 0400360201 & $1.54\pm0.05$ & & & & & 281/265 & & & & & & & & &\\
 & 0400360301 & $1.50\pm0.6$ & & & & & 195/203 & & & & & & & & &\\
 & 0400360601 & $1.61\pm0.05$ & & & & & 157/173 & $8.03\pm0.03$ & 10 & $\rm -85^{+27}_{-33}$ & $+0.141\pm0.003$ & 13.4 & 99.96\% & 99\% & Ly$\alpha$ & $\rm -110^{+53}_{-61}$\\
 & 0400360801 & $1.54\pm0.05$ & & $6.42\pm0.03$ & 100 & $\rm 151^{+63}_{-60}$ & 181/203 & & & & & & & & &\\
Mrk~205 & 0124110101 & $1.71\pm0.04$ & & $6.37\pm0.04$ & 100 & $100\pm43$ & 309/314 & $7.70\pm0.03$ & 10 & $-50\pm18$ & $+0.100\pm0.004$ & 11 & 99.7\% & 96.9\% & Ly$\alpha$ & $+37\pm33$\\
 & & & & $6.86\pm0.05$ & 100 & $90\pm49$ & & & & & & & & & &\\
 & 0401240201 & $1.79\pm0.04$ & & $6.34\pm0.02$ & 10 & $70\pm27$ & 465/392 & & & & & & & & &\\
 & 0401240501 & $1.85\pm0.02$ & & $6.55\pm0.04$ & 100 & $65\pm29$ & 553/603 & & & & & & & & &\\
Mrk~590 & 0201020201 & $1.52\pm0.03$ & & $6.42\pm0.01$ & 10 & $110\pm21$ & 739/776 & & & & & & & & &\\
H~557-385 & 0404260101 & $1.20\pm0.06$ & $21\pm2$ & $6.42\pm0.01$ & 100 & $370\pm67$ & 231/202 & & & & & & & & & \\
 & 0404260301 & $1.14\pm0.05$ & $21\pm2$ & $6.44\pm0.01$ & 100 & $460\pm55$ & 409/337& & & & & & & & &\\
 & & & & $6.90\pm0.02$ & 100 & $\rm 189^{+47}_{-41}$ & & & & & & & & & &\\
TON~S180 & 0110890401 & $2.05\pm0.05$ & & & & & 174/178 & & & & & & & & &\\
 & 0110890701 & $1.96\pm0.08$ & & & & & 123/104 & & & & & & & & &\\
PG~1211+143 & 0112610101 & $2.80\pm0.12$ & $11.7\pm1.5$ & $6.52\pm0.05$ & 100 & $100\pm43$ & 307/273 & $7.62\pm0.02$ & 100 & $\rm -130^{+18}_{-24}$ & $+0.128\pm0.003$ & 56 & $>$$99.99$\%  & $>99.9$\%  & He$\alpha$ & $\rm -128^{+32}_{-60}$\\
 & 0208020101 & $1.71\pm0.05$ & & $6.52\pm0.03$ & 100 & $\rm 135^{+60}_{-51}$ & 219/200 & & & & & & & & &\\
 & 0502050101 & $2.07\pm0.04$ & & $6.36\pm0.03$ & 100 & $141\pm46$ & 258/291 & & & & & & & & &\\
 & 0502050201 & $2.06\pm0.05$ & & $6.36\pm0.06$ & 100 & $\rm 90^{+53}_{-50}$ & 237/211 & & & & & & & & & \\
Ark~564 & 0206400101 & $2.45\pm0.02$ & & $6.34\pm0.04$ & 100 & $35\pm18$ & 829/900 & & & & & & & & &\\
 & & & & $6.71\pm0.03$ & 100 & $50\pm18$ & & & & & & & & & &\\
& & & & & & & & & & & & & & & &\\ 
%\hline\\[-6.5pt] 
\multicolumn{17}{c}{Type~2 Sources}\\[1.2pt]
%\hline
 & & & & & & & & & & & & & & & &\\ 
MCG-5-23-16 & 0112830401 & $1.61\pm0.03$ & $2.5\pm0.4$ & $6.37\pm0.01$ & 100 & $90\pm15$ & 1081/1123 & & & & & & & & &\\
 & 0302850201 & $1.53\pm0.01$ & $1.2\pm0.2$ & $6.41\pm0.01$ & 100 & $90\pm6$ & 1554/1391 & $7.84\pm0.04$ & 100 & $-18\pm4$ & $+0.118\pm0.005$ & 22.6 & 99.996\% & $>99.9$\% & Ly$\alpha$ & $-9\pm5$\\
 & & & & $6.93\pm0.02$ & 100 & $26\pm7$ & & & & & & & & & &\\
NGC~5506 & 0013140101 & $1.68\pm0.04$ & $2.8\pm0.5$ & $6.44\pm0.01$ & 100 & $\rm 125^{+21}_{-18}$ & 1049/960 & & & & & & & & &\\
 & 0201830201 & $1.79\pm0.04$ & $3.4\pm0.4$ & $6.39\pm0.01$ & 100 & $110\pm18$ & 1060/1002 & & & & & & & & &\\
 & 0201830301 & $1.88\pm0.03$ & $4.7\pm0.5$ & $6.39\pm0.01$ & 100 & $120\pm18$ & 1116/984 & & & & & & & & &\\
 & 0201830401 & $1.93\pm0.04$ & $4.8\pm0.5$ & $6.41\pm0.01$ & 100 & $130\pm18$ & 931/948 & & & & & & & & &\\
 & 0201830501 & $1.93\pm0.03$ & $4.2\pm0.4$ & $6.41\pm0.02$ & 100 & $85\pm15$ & 1115/1082 & & & & & & & & &\\
NGC~7172 & 0147920601 & $1.70\pm0.06$ & $9.9\pm0.9$ & $6.40\pm0.02$ & 100 & $\rm 110^{+36}_{-30}$ & 411/455 & & & & & & & & &\\
 & 0414580101 & $1.72\pm0.03$ & $9.0\pm0.4$ & $6.39\pm0.01$ & 100 & $80\pm12$ & 1135/1128 & & & & & & & & &\\
NGC~7314 & 0111790101 & $1.97\pm0.04$ & $1.8\pm0.4$ & $6.42\pm0.02$ & 100 & $70\pm18$ & 916/1006 & & & & & & & & &\\
NGC~2110 & 0145670101 & $1.59\pm0.04$ & $4.7\pm0.5$ & $6.43\pm0.01$ & 100 & $\rm 150^{+18}_{-24}$ & 903/954 & & & & & & & & &\\
NGC~4507 & 0006220201 & $1.50\pm0.06$ & $38.0\pm0.5$ & $6.37\pm0.01$ & $\rm 76^{+10}_{-12}$ & $227\pm26$ & 649/682 & $8.32\pm0.02$ & 10 & $-35\pm12$ & $+0.177\pm0.002$ & 12.5 & 99.9\% & 98.7\% & Ly$\alpha$ & $-18\pm21$\\
 & & & & $6.90\pm0.04$ & 100 & $36\pm20$ & & & & & & & & & &\\
NGC~7582 & 0112310201 & $0.80\pm0.06$ & $19.0\pm2.4$ & $6.39\pm0.01$ & 100 & $\rm 425^{+113}_{-73}$ & 168/149 & $8.99\pm0.04$ & 10 & $\rm -91^{+29}_{-41}$ & $+0.255\pm0.003$ & 12 & 99.5\% & 98.2\% & He$\alpha$ & $\rm -124^{+107}_{-119}$\\
 & & & & $7.02\pm0.05$ & 100 & $\rm 143^{+74}_{-68}$ & & & & & & & & & &\\
 & 0204610101 & $0.50\pm0.06$ & $\rm 9.6^{+1.2}_{-2.1}$ & $6.41\pm0.05$ & 100 & $\rm 940^{+122}_{-85}$ & 317/287 & & & & & & & & &\\
 & & & & $6.91\pm0.02$ & 100 & $290\pm61$ & & & & & & & & & &\\
 & & & & & & & & & & & & & & & &\\
\hline
\end{tabular}
  \tablefoot{The baseline models are composed by a simple absorbed power-law continuum with narrow Gaussian emission lines. 
The narrow absorption lines refer to those that have been detected in the $E=6.4{-}7.1$~keV band with F-test confidence levels greater than 99\% and to those detected at energies greater than 7.1~keV with additional Monte~Carlo probability $\ge$95\%. The errors are at the 1$\sigma$ level.\\
\tablefoottext{1}{Source name.} 
\tablefoottext{2}{\mbox{{\it~XMM-Newton}} observation ID.} 
\tablefoottext{3}{Power-law continuum photon index.} 
\tablefoottext{4}{Neutral absorber equivalent Hydrogen column density.} 
\tablefoottext{5}{Gaussian emission line rest-frame energy.} 
\tablefoottext{6}{Emission line width.} 
\tablefoottext{7}{Emission line equivalent width.} 
\tablefoottext{8}{Best-fit $\chi^2$ and degrees of freedom $\nu$ of the baseline model.} 
\tablefoottext{9}{Absorption line rest-frame energy.} 
\tablefoottext{10}{ Absorption line width.} 
\tablefoottext{11}{Absorption line equivalent width.} 
\tablefoottext{12}{Absorption line blue-shifted velocity.} 
\tablefoottext{13}{$\Delta\chi^2$ relative to the addition of the absorption line.}
\tablefoottext{14}{Detection confidence level from the F-test.}
\tablefoottext{15}{ Detection confidence level from extensive Monte~Carlo simulations.} 
\tablefoottext{16}{Absorption line identification as Fe~XXV 1s$^2$--1s2p (He$\alpha$), Fe~XXV 1s$^2$--1s3p (He$\beta$), Fe~XXVI 1s$-$2p (Ly$\alpha$) or Fe~XXVI 1s$-$3p (Ly$\beta$).} 
\tablefoottext{17}{Consistency check of the $EW$ of the absorption line with the MOS cameras.}\\
\tablefoottext{a}{Only MOS1 data available.}
\tablefoottext{b}{Only MOS2 data available.}}
\end{table}