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Table A.3:

Estimates of the mean Fe K absorption line parameters for the sample sources among the  XMM-Newton observations in which they have been detected.

Source 		Fe XXV He$\alpha $ $v_{\rm out}$ Fe XXV He$\beta $ $v_{\rm out}$ Fe XXVI Ly$\alpha $ $v_{\rm out}$ Fe XXVI Ly$\beta $ $v_{\rm out}$ $\langle v_{\rm out}\rangle$
  (eV) (c) (eV) (c) (eV) (c) (eV) (c) (c)
1 2 3 4 5 6 7 8 9 10
                   
NGC 4151         $-32\pm7$ $+0.105\pm0.005$     +0.105
IC4329A         $-10\pm3$ $+0.098\pm0.003$     +0.098
NGC 3783 $\rm -14(^{-10}_{-17})$ $\rm -0.009(^{-0.004}_{-0.013})$ $-25\pm7$ $-0.018\pm0.004$         -0.013
NGC 3516 $\rm -20(^{-15}_{-25})$ $\rm +0.004(^{+0.011}_{-0.001})$ $-33\pm9$ $+0.009\pm0.002$ $\rm -23(^{-21}_{-27})$ $\rm +0.013(^{+0.017}_{+0.008})$ $-34\pm9$ $+0.004\pm0.004$ +0.008
Mrk 509         $\rm -23(^{-19}_{-32})$ $\rm +0.170(^{+0.196}_{+0.141})$     +0.170
Ark 120         $-25\pm9$ $+0.269\pm0.002$     +0.269
Mrk 279 $-19\pm9$ $-0.001\pm0.004$             -0.001
Mrk 79         $-43\pm14$ $+0.091\pm0.004$     +0.091
NGC 4051         $\rm -58(^{-19}_{-96})$ $\rm +0.084(^{+0.150}_{+0.018})$     +0.084
Mrk 766         $\rm -33(^{-27}_{-39})$ $\rm +0.067(^{+0.091}_{+0.044})$     +0.067
Mrk 841         $-46\pm16$ $+0.034\pm0.003$     +0.034
ESO 323+G77 $-78\pm13$ $+0.005\pm0.002$     $-77\pm15$ $+0.008\pm0.003$     +0.007
1H419-577         $\rm -55^{+18}_{-21}$ $+0.037\pm0.005$     +0.037
Mrk 290         $\rm -85^{+27}_{-33}$ $+0.141\pm0.003$     +0.141
Mrk 205         $-50\pm18$ $+0.100\pm0.004$     +0.100
PG 1211+143 $\rm -130^{+18}_{-24}$ $+0.128\pm0.003$             +0.128
MCG-5-23-16         $-18\pm4$ $+0.118\pm0.005$     +0.118
NGC 4507         $-35\pm12$ $+0.177\pm0.002$     +0.177
NGC 7582 $\rm -91^{+29}_{-41}$ $+0.255\pm0.003$             +0.255

Notes. For the sources with multiple line detections in different  XMM-Newton observations we report also the lowest and highest values of the EW and blue-shifted velocity within brackets. Instead, if there is only one line detection we report the associated 1$\sigma $ errors.
(1) Source name. (2, 3) Mean EW and blue-shifted velocity for Fe XXV He$\alpha $. (4, 5) Mean EW and blue-shifted velocity for Fe XXV He$\beta $. (6, 7) Mean EW and blue-shifted velocity for Fe XXVI Ly$\alpha $. (8, 9) Mean EW and blue-shifted velocity for Fe XXVI Ly$\beta $. (10) Mean blue-shifted velocity from all the Fe K absorption lines.


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