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Table 2:

Properties of the sources in the sample. The analysed XMM- Newton observations are indicated by the revolution number.
Sources RXTE z $\langle$Log ( $M_{\rm BH}$/$M_{\odot}$)$\rangle$ $\langle T_{\rm orb}$(10$r_{\rm g}$)$\rangle$ Ref. Rev. Num. $F_{2{-}10~\rm keV}$ Obs. Duration $\Delta t$ $\Delta E$ FOM $\Gamma$ $N_{\rm H}$
  (cts/s)     (ks)     (10-11 erg cm-2 s-1) (ks) (ks) (keV) (10-11 erg cm-2 s-1)   (1022 cm-2)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
IC 4329a 7.29 0.0161 7.29 19 1, 2, 3, 4 210 15.3 10 2.5 0.1 8.0 $\rm 2.04^{+0.16}_{-0.08}$ $\rm 2.66^{+2.13}_{-2.27}$
            670 9.48 133 2.5 0.1 65.8 $\rm 1.73^{+0.03}_{-0.04}$ $\rm0.35^{+0.67}_{-0.16}$
MCG -5-23-16 6.46 0.0085 7.60 39 13 363 7.43 22 2.5 0.1 4.2 $\rm 1.69^{+0.10}_{-0.13}$ <3.50
            1099 8.29 122 2.5 0.1 25.9 $\rm 1.79^{+0.03}_{-0.06}$ $\rm 2.67^{+0.50}_{-0.94}$
NGC 3783 4.90 0.0097 7.01 10 1, 2, 3, 4, 5 193 5.27 37 2.5 0.1 19.7 $\rm 1.86^{+0.05}_{-0.06}$ $\rm 2.80^{+0.57}_{-0.95}$
            371 3.96 131 2.5 0.1 52.3 1.67 $\pm$ 0.20 $1.61\pm 1.10$
            372 5.56 136 2.5 0.1 76.3 $\rm 1.82^{+0.03}_{-0.07}$ $\rm 2.56^{+0.50}_{-0.70}$
NGC 5548 3.58 0.0170 7.71 50 1, 2, 3, 4, 5 191 3.14 23 2.5 0.1 1.4 $\rm 1.67^{+0.11}_{-0.06}$ <1.54
            290 3.86 93 2.5 0.1 7.1 $1.77\pm0.07$ <1.83
            291 4.89 37 2.5 0.1 3.6 $1.89\pm0.10$ $\rm 2.13^{+1.36}_{-1.30}$
NGC 3516 3.21 0.0088 7.21 16 1, 2, 3, 5 245 2.34 129 5.0 0.1 19.2 $1.81\pm0.09$ $\rm 5.32^{+1.16}_{-1.17}$
            352 1.53 128 5.0 0.1 12.4 $\rm 1.82^{+0.11}_{-0.17}$ $\rm 7.82^{+1.24}_{-1.39}$
            1250 5.24 52 2.5 0.1 17.3 $\rm 2.15^{+0.06}_{-0.09}$ $\rm 4.76^{+0.75}_{-1.23}$
            1251 4.60 69 2.5 0.1 20.1 $\rm 2.21^{+0.06}_{-0.07}$ $\rm 6.07^{+0.96}_{-0.93}$
            1252 3.64 68 2.5 0.1 15.7 $\rm 2.29^{+0.09}_{-0.08}$ $\rm 8.62^{+1.12}_{-0.95}$
            1253 4.48 68 2.5 0.1 19.3 $\rm 2.26^{+0.07}_{-0.15}$ $\rm 6.41^{+1.14}_{-1.15}$
MRK 509 3.12 0.0344 7.84 68 1, 2, 3, 4, 5 161 2.97 30 2.5 0.1 1.3 $\rm 1.63^{+0.13}_{-0.11}$ <3.04
            250 3.84 43 2.5 0.1 2.4 $\rm 1.72^{+0.10}_{-0.15}$ <2.73
            1073 3.67 85 2.5 0.1 4.6 $1.69\pm0.03$ <0.59
            1074 3.70 46 2.5 0.1 2.5 $\rm 1.74^{+0.09}_{-0.02}$ <0.72
            1168 4.26 69 2.5 0.1 4.4 $\rm 1.71^{+0.08}_{-0.05}$ <0.69
MCG -6-30-15 3.08 0.0077 5.84 0.67 3, 8 108A 2.62 43 2.5 0.1 168.0 $\rm 2.01^{+0.19}_{-0.32}$ <1.56
            108B 3.60 55 2.5 0.1 295.3 2.50 $\pm$ 0.08 7.30 $\pm$ 1.14
            301 4.11 84 2.5 0.1 514.9 2.47 $\pm$ 0.05 6.77 $\pm$ 0.90
            302 4.53 127 2.5 0.1 858.1 $\rm 2.28^{+0.06}_{-0.04}$ $\pm$0.70
            303 4.01 125 2.5 0.1 747.6 $\rm 2.17^{+0.29}_{-0.19}$ $\rm 1.37^{+0.80}_{-0.87}$
MCG +8-11-11 2.36 0.0205 7.18 15 3 794 4.52 38 2.5 0.1 11.6 $\rm 1.64^{+0.09}_{-0.07}$ <1.84
NGC 7314 2.16 0.0048 6.67 4.6 12 256 3.93 43 2.5 0.1 36.9 2.12 $\pm$ 0.09 $\rm 2.68^{+1.25}_{-1.27}$
            1172 1.54 82 5.0 0.1 27.5 $\rm 1.94^{+0.14}_{-0.11}$ $\rm 3.84^{+1.85}_{-1.44}$
AKN 120 2.14 0.0323 8.14 134 1, 2, 3, 4, 5 679 3.76 112 2.5 0.1 3.1 $\rm 1.97^{+0.06}_{-0.07}$ $\rm 1.03^{+0.73}_{-0.99}$
MRK 279 2.13 0.0305 7.79 60 1, 2, 3, 5 1087 2.60 59 5.0 0.1 2.6 $\rm 1.91^{+0.06}_{-0.09}$ <2.38
            1088 2.43 59 5.0 0.1 2.4 $\rm 1.75^{+0.05}_{-0.10}$ <2.07
            1089 2.38 38 5.0 0.1 1.5 $\rm 2.03^{+0.08}_{-0.15}$ $\rm 4.20^{+2.06}_{-2.00}$
MR 2251-178 2.10 0.0640 8.40 246 10 447 2.03 64 5.0 0.1 0.5 1.61 $\pm$ 0.09 <2.14
NGC 3227 2.10 0.0039 7.39 24 1, 2, 3, 4, 5 178 0.85 35 5.0 0.1 1.2 $\rm 1.63^{+0.20}_{-0.13}$ $\rm 7.84^{+2.75}_{-2.04}$
            1279 3.64 106 2.5 0.1 16.1 1.92 $\pm$ 0.08 $\rm 2.89^{+1.08}_{-1.15}$
IRAS 05078+1626 2.08 0.0179 7.04 11 1 1410 2.41 58 5.0 0.1 13.0 $\rm 1.78^{+0.10}_{-0.09}$ $\rm 2.53^{+1.46}_{-1.25}$
MRK 590 1.95 0.0264 7.37 23 1, 2, 4, 5 837 0.56 108 9.0 0.1 2.6 $\rm 2.30^{+0.37}_{-0.15}$ $\rm 5.21^{+4.66}_{-1.97}$
MRK 766 1.77 0.0129 5.92 0.82 3 82 1.52 39 5.0 0.1 72.7 $\rm 2.25^{+0.17}_{-0.16}$ 3.46 $\pm$ 2.29
            265 2.44 129 5.0 0.1 386.0 $\rm 2.10^{+0.08}_{-0.04}$ <1.20
            999 0.72 95 8.0 0.1 83.9 $\rm 1.85^{+0.23}_{-0.32}$ $\rm 5.13^{+2.54}_{-2.30}$
            1000 1.13 98 6.5 0.1 135.8 $\rm 1.99^{+0.20}_{-0.07}$ <2.77
            1001 1.40 98 6.0 0.1 168.3 $\rm 2.13^{+0.11}_{-0.12}$ <2.92
            1002 1.74 95 5.0 0.1 202.7 $\rm 2.27^{+0.10}_{-0.11}$ $\rm 3.59^{+1.23}_{-1.46}$
            1003 1.48 98 5.5 0.1 177.9 $\rm 2.01^{+0.17}_{-0.04}$ <2.23
            1004 1.30 35 5.0 0.1 55.8 $\rm 2.10^{+0.15}_{-0.08}$ <5.06
NGC 7469 1.69 0.0164 7.14 13 1, 2, 3, 4, 5 192A 2.49 18 5.0 0.1 3.4 $\rm 1.88^{+0.17}_{-0.15}$ <3.97
            192B 2.66 23 5.0 0.1 4.6 $\rm 1.79^{+0.11}_{-0.05}$ <1.18
            912 2.83 85 2.5 0.1 18.0 $\rm 1.92^{+0.08}_{-0.07}$ $\rm 1.55^{+1.18}_{-0.93}$
            913 2.93 79 2.5 0.1 17.3 $\rm 1.97^{+0.07}_{-0.08}$ 2.24 $\pm$ 1.09
MCG -2-58-22 1.61 0.0469 8.00 99 1, 3 180 3.02 10 2.5 0.1 0.3 $\rm 1.68^{+0.22}_{-0.15}$ <4.04
NGC 526A 1.61 0.0191 6.98 9 1,13 647 2.20 44 2.5 0.1 10.5 $\rm 1.61^{+0.05}_{-0.12}$ $\rm 2.56^{+1.30}_{-1.44}$
NGC 4051 1.49 0.0023 5.90 0.77 2, 3, 4 263 2.35 117 5.5 0.1 355.8 $\rm 2.20^{+0.09}_{-0.07}$ $\rm 2.86^{+1.07}_{-1.10}$
            541 0.56 50 6.0 0.2 36.2 $\rm 1.56^{+0.23}_{-0.31}$ <4.35
ESO 141-G055 1.37 0.0360 7.51 31 1 1435 A 2.82 20 5.0 0.1 1.8 $\rm 2.06^{+0.21}_{-0.15}$ <3.88
            1435 B 2.54 21 5.0 0.1 1.7 $\rm 2.15^{+0.23}_{-0.21}$ <5.42
            1436 2.31 41 5.0 0.1 3.0 $\rm 2.10^{+0.19}_{-0.13}$ <3.31
            1445 2.88 78 5.0 0.1 7.2 $\rm 1.94^{+0.06}_{-0.08}$ <0.78
UGC 3973 1.32 0.0222 7.74 54 1, 2, 4, 5 1247 2.33 21 5.0 0.1 0.9 $\rm 2.02^{+0.18}_{-0.17}$ <4.65
          1263 2.01 20 5.0 0.1 0.7 $\rm 1.64^{+0.16}_{-0.09}$ <3.17
          1332 1.84 20 5.0 0.1 0.7 $\rm 1.63^{+0.23}_{-0.13}$ <4.25
          1535 0.77 87 6.0 0.1 1.2 $\rm 1.70^{+0.11}_{-0.20}$ $\rm 5.87^{+3.32}_{-1.37}$
Fairall 9 1.25 0.0470 8.00 98 1, 2, 3, 4, 5 105 1.16 29 5.0 0.1 0.3 $\rm 1.73^{+0.19}_{-0.16}$ <5.00
ESO 198-G024 1.21 0.0455 8.38 235 1, 9 207 1.30 31 5.0 0.1 0.2 $\rm 1.84^{+0.16}_{-0.15}$ <3.43
            1128 1.02 122 6.0 0.1 0.5 $\rm 1.75^{+0.19}_{-0.09}$ $\rm 1.83^{+1.78}_{-1.22}$
MRK 110 1.17 0.0353 6.99 9.5 2, 3, 4, 5 904 2.80 47 2.5 0.1 13.8 1.87 $\pm$ 0.10 $\rm 1.79^{+1.38}_{-1.36}$
AKN 564 1.13 0.0247 6.24 1.7 3, 7 930 1.60 99 5.0 0.2 94.1 $\rm 2.50^{+0.11}_{-0.04}$ <1.28
NGC 7213 1.12 0.0058 8.04 107 1, 11 269 2.16 42 5.0 0.1 0.9 $\rm 1.69^{+0.10}_{-0.03}$ <0.85
ESO 511-G030 1.10 0.0224 8.66 448 6 1402 1.93 109 5.0 0.1 0.5 1.89 $\pm$ 0.08 $\rm 2.03^{+1.15}_{-1.07}$
MRK 704 1.06 0.0292 7.55 35 1 1074 0.99 21 5.0 0.2 0.6 $\rm 1.88^{+0.40}_{-0.17}$ $\rm 6.58^{+5.44}_{-2.47}$
            1630 1.07 98 5.5 0.1 3.0 $\rm 1.87^{+0.19}_{-0.08}$ <3.57
NGC 4593 1.05 0.0047 6.91 7.9 1, 2, 3, 5 465 4.00 76 2.5 0.1 38.5 $\rm 1.84^{+0.06}_{-0.03}$ $\rm 1.21^{+0.91}_{-0.93}$

Columns: (2) RXTE count rate; (5) estimated Keplerian orbital period at r=10 $r_{\rm g}$; (6) references for the mass estimates.; (10) and (11) chosen time and energy resolutions for the excess map analysis; (12) FOM value (see Sect. 4); References: (1) Wang & Zhang (2007); (2) Peterson et al. (2004); (3) Bian & Zhao (2003); (4) Kaspi et al. (2000); (5) Ho (1998); (6) Winter et al. (2008); (7) Botte et al. (2004); (8) Vaughan et al. (2003); (9) Rokaki & Boisson (1999); (10) Brunner et al. (1997); (11) Nelson & Whittle (1995); (12) Padovani & Rafanelli (1988); (13) Wandel & Mushotzky (1986).


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