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Table A.2:

Best-fit parameters of the baseline models and absorption lines for the type 1 and type 2 sources.
Source OBSID Baseline model Absorption line
    $\Gamma$ $N_{\rm H}$ E $\sigma $ EW $\chi^2/\nu$ E $\sigma $ EW $v_{\rm out}$ $\Delta \chi ^2$ F-test M.C. ID EW $_{{\rm MOS}}$
      (1022 cm-2) (keV) (eV) (eV)   (keV) (eV) (eV) (c)         (eV)
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17
Type 1 Sources
                                 
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 $ $+10\pm21$
  0112210201b $1.66\pm0.02$ $1.9\pm0.2$ $6.39\pm0.01$ 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 $57\pm11$                    
  0112210501b $1.74\pm0.02$ $2.2\pm0.2$ $6.39\pm0.01$ 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 0147190101b $1.86\pm0.01$   $6.39\pm0.01$ 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                  
  0302480501a $1.71\pm0.02$   $6.43\pm0.01$ 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 0109141401b $2.04\pm0.03$ $1.7\pm0.4$ $6.39\pm0.01$ 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                  
  0205340401a $1.61\pm0.04$   $6.49\pm0.03$ 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 $50\pm18$                    
Type 2 Sources
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 $290\pm61$                    

Notes. 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.
(1) Source name. (2)  XMM-Newton observation ID. (3) Power-law continuum photon index. (4) Neutral absorber equivalent Hydrogen column density. (5) Gaussian emission line rest-frame energy. (6) Emission line width. (7) Emission line equivalent width. (8) Best-fit $\chi^2$ and degrees of freedom $\nu$ of the baseline model. (9) Absorption line rest-frame energy. (10)  Absorption line width. (11) Absorption line equivalent width. (12) Absorption line blue-shifted velocity. (13)  $\Delta \chi ^2$ relative to the addition of the absorption line. (14) Detection confidence level from the F-test. (15)  Detection confidence level from extensive Monte Carlo simulations. (16) Absorption line identification as Fe XXV 1s2-1s2p (He$\alpha $), Fe XXV 1s2-1s3p (He$\beta $), Fe XXVI 1s-2p (Ly$\alpha $) or Fe XXVI 1s-3p (Ly$\beta $). (17) Consistency check of the EW of the absorption line with the MOS cameras.
(a) Only MOS1 data available. (b) Only MOS2 data available.


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