Table 2: Multi-wavelength luminosities and $M_{\rm BH}$ of the total X-ray sample.
Name Class Sat Log $F_{2-10 ~{\rm keV}}$ Log $L_{2-10~{\rm keV}}$ Ref. CThick Log $L_{\rm [OIII]}$ Log $L_{\rm H\alpha}$ Log $M_{\rm BH}$ Method Ref.
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
NGC 676 S2: X -13.62 40.79 1 $\surd$ 39.04 38.62 - - -
NGC 1058 S2 C <-14.42 <37.55 2 ? 37.90 38.16 4.88 I$_{\sigma}$ 8
NGC 1068 S1.9 X -11.31 42.84 1 $\surd$ 41.91 41.53 7.20 M 1
NGC 1167 S2 A -13.39 42.07 3 $\surd$ 40.76 40.81 - - -
NGC 1275 S1.5 X -10.91 42.83 2 $\times$ 41.91 42.07 8.51 I$_{\sigma}$ 2
NGC 1667 S2 A -13.1 42.31 3 $\surd$ 40.42 40.17 7.88 I$_{\sigma}$ 2
NGC 2273 S2 A -12.16 42.58 4 $\surd$ 40.94 40.92 7.30 I$_{\sigma}$ 2
NGC 2639 S1.9 A -12.49 40.82 5 ? 40.40 40.56 8.02 I$_{\sigma}$ 9
NGC 2655 S2 A -10.98 41.85 5 $\times$ 39.92 40.03 7.77 I$_{\sigma}$ 9
NGC 2683 L2/S2 C -13.62 38.21 2 ? 38.58 37.69 7.51 I$_{\sigma}$ 9
NGC 2685 S2/T2: X :-12.53 39.94 1 $\times$ 38.96 39.21 7.15 I$_{\sigma}$ 9
NGC 3031 S1.5 X -10.89 40.25 1 $\times$ 38.56 38.94 7.80 S 1
NGC 3079 S2 C -11.69 42.62 2 $\surd$ 40.07 40.89 7.65 I$_{\sigma}$ 3
NGC 3147 S2 C -11.39 41.89 2 $\times$ 40.07 40.01 8.79 I$_{\sigma}$ 3
NGC 3185 S2: X -13.7 40.79 1 $\surd$ 39.90 40.07 6.06 I$_{\sigma}$ 2
NGC 3227 S1.5 X -10.94 41.74 1 $\times$ 40.51 40.20 7.59 R 4
NGC 3486 S2 X -12.93 38.86 1 ? 37.99 37.85 6.14 I$_{\sigma}$ 8
NGC 3489 T2/S2 C <-13.57 <39.88 2 $\surd$ 38.86 38.48 7.48 I$_{\sigma}$ 5
NGC 3516 S1.2 C -10.87 42.29 2 $\times$ 40.50 39.91 7.36 R 1
NGC 3608 L2/S2 C -13.69 39.10 2 $\times$ 38.22 38.23 8.04 S 1
NGC 3627 T2/S2 C <-13.81 <37.88 2 ? 38.79 39.35 7.99 I$_{\sigma}$ 5
NGC 3941 S2: X -13.35 38.88 1 $\times$ 38.63 38.78 8.15 I$_{\sigma}$ 7
NGC 3982 S1.9 A -13.28 41.18 2 $\surd$ 40.50 39.87 6.09 I$_{\sigma}$ 2
NGC 4051 S1.2 C -11.2 41.31 2 $\times$ 39.81 39.68 6.11 R 4
NGC 4138 S1.9 X -11.04 41.29 1 $\times$ 38.74 38.69 7.75 I$_{\sigma}$ 9
NGC 4151 S1.5 X -10.2 42.47 1 $\times$ 41.47 40.94 7.18 R 4
NGC 4168 S1.9: X -13.19 39.87 1 $\times$ 38.46 38.93 7.95 I$_{\sigma}$ 6
NGC 4235 S1.2 A -10.92 42.22 2 $\times$ 40.41 40.97 - - -
NGC 4258 S1.9 C -10.91 40.86 2 $\times$ 39.07 38.65 7.61 M 1
NGC 4388 S1.9 C -10.78 41.72 2 $\times$ 40.54 40.26 6.80 I$_{\sigma}$ 3
NGC 4395 S1 X -11.07 39.81 1 $\times$ 38.28 38.53 5.04 S 1
NGC 4472 S2:: C <-13.18 <39.32 2 $\times$ <37.81 <37.59 8.80 I$_{\sigma}$ 6
NGC 4477 S2 X -12.85 39.65 1 $\times$ 39.04 39.06 7.92 I$_{\sigma}$ 9
NGC 4501 S1.9 X -12.91 39.59 1 $\times$ 39.23 39.06 7.90 I$_{\sigma}$ 3
NGC 4565 S1.9 X -12.6 39.43 1 $\times$ 38.69 38.72 7.70 I$_{\sigma}$ 3
NGC 4579 S1 C -11.47 41.03 6 $\times$ 39.42 39.72 7.78 I$_{\sigma}$ 3
NGC 4639 S1.0 X -12.55 40.22 1 $\times$ 38.71 39.90 6.85 I$_{\sigma}$ 8
NGC 4698 S2 X -13.34 39.16 1 $\times$ 38.86 38.74 7.84 I$_{\sigma}$ 9
NGC 4725 S2: X -13.4 38.89 1 $\times$ 38.58 38.24 7.49 I$_{\sigma}$ 3
NGC 5033 S1.5 X -11.52 41.08 1 $\times$ 39.72 40.42 7.30 I$_{\sigma}$ 3
NGC 5194 S2 C -12.77 40.91 2 $\surd$ 39.90 39.87 6.95 I$_{\sigma}$ 2
NGC 5273 S1.5 X -11.13 41.36 1 $\times$ 39.03 38.48 6.51 I$_{\sigma}$ 2
NGC 5548 S1.5 X -10.5 43.25 2 $\times$ 41.16 40.26 8.03 I$_{\sigma}$ 4
NGC 6482 T2/S2 C -13.33 40.16 2 $\times$ - 39.26 8.75 I$_{\sigma}$ 9
NGC 6503 T2/S2 C -14.39 37.10 2 ? - 37.41 5.56 I$_{\sigma}$ 8
NGC 7479 S1.9 X -11.95 41.12 2 ? 40.25 40.67 7.07 I$_{\sigma}$ 9
NGC 7743 S2 A -13.14 41.47 5 $\surd$ 40.21 40.24 6.59 I$_{\sigma}$ 2
Notes: Col. (1): galaxy name; Col. (2): optical classification; Col. (3): Satellite used: "C''=Chandra, "X''=XMM-Newton, "A''=ASCA; Col. (4): logarithm of the 2-10 keV flux in units of erg cm-2 s-1, not corrected for Compton thick candidates. Col. (5): logarithm of the 2-10 keV luminosity, corrected for Compton thick candidates. Col. (6): X-RAY REFERENCES: (1) Cappi et al. (2006); (2) this work; (3) Pappa et al. (2001); (4) Guainazzi et al. (2005); (5) Terashima et al. (2002); (6) Eracleous et al. (2002); Col. (7): Final classification: "$\surd$''=Compton thick candidates, "$\times$''=Compton thin candidate and "?''=doubtful objects.; Col. (8): logarithm of the [OIII] $_{\lambda 5007}$luminosity corrected for Galactic absorption and NLR extinction; Col. (9): logarithm of the H${\alpha}$ (broad+narrow component) luminosity corrected for Galactic absorption and NLR extinction; Col. (10): logarithm of the $M_{\rm BH}$ value in units of $M_{\odot}$; Col. (11): $M_{\rm BH}$ measurement methods; M: maser kinematics; G: gas kinematics; S: stellar kinematics; R: reverberation mapping; I$_{\sigma}$: inferred from the mass-velocity dispersion correlation; Col. (12): $M_{\rm BH}$ references: (1) Ho (2002); (2) Woo & Urry (2002); (3) Merloni et al. (2003); (4) Kaspi et al. (2000); (5) Pellegrini (2005); (6) Merritt & Ferrarese (2001); (7) di Nella et al. (1995); (8) Barth et al. (2002); (9) McElroy (1995).

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