Table 1: Sources used in this paper. Column 1 lists the names of the sources and Col. 2 gives the distance used to derive the luminosities from the fluxes. The black hole mass was calculated from the velocity dispersion relation Merritt & Ferrarese (2001). Columns 4 and 5 give the measured radio and X-ray fluxes. For the LLAGN sample we only list the radio luminosity as directly taken from the original paper. The last two columns give the radio luminosity and the equivalent X-ray luminosity as described in Eq. (7). This luminosity has also been corrected for the different observed energy bands assuming a photon index of 1.6.
Type/name Distance $M_{\rm {BH}}$ ${F}_{\rm {5~GHz}}$ ${F}_{\rm {2{-}10~keV}} $ $\nu {L}_{\rm {5~GHz}} $ ${L'}_{\rm {3{-}9~keV}} $
[Mpc] $[M_\odot]$ [mJy] $\left[\mbox{erg}/\mbox{s}\right]$ $\left[\mbox{erg}/\mbox{s}\right]$ $\left[\mbox{erg}/\mbox{s}\right]$
SGR A*            
Quiet 0.008 $3.\times{10}^6$ 600. $2.2\times10^{33}$ $2.3\times{10}^{32} $ $ 6.3\times{10}^{37}$
Flare 0.008 $3.\times{10}^6$ 600. $1.0\times10^{35}$ $2.3\times{10}^{32} $ $ 2.87\times{10}^{39}$
LLAGN            
NGC 2787 13.3 $1.7\times{10}^8$   $2.5\times{10}^{-14}$ $1.66\times{10}^{37}$ $ 3.93\times{10}^{44}$
NGC 3147 40.9 $6.58\times{10}^8$   $3.7\times{10}^{-12}$ $1.02\times{10}^{38}$ $ 1.65\times{10}^{48}$
NGC 3169 19.7 $6.21\times{10}^7$   $2.45\times{10}^{-12}$ $1.55\times{10}^{37}$ $ 3.76\times{10}^{46}$
NGC 3226 23.4 $1.39\times{10}^8$   $7.6\times{10}^{-13}$ $1.58\times{10}^{37}$ $ 3.15\times{10}^{46}$
NGC 4143 17. $3.1\times{10}^8$   $3.1\times{10}^{-13}$ $1.45\times{10}^{37}$ $ 1.3\times{10}^{46}$
NGC 4278 9.7 $4.5\times{10}^8$   $8.1\times{10}^{-13}$ $8.13\times{10}^{37}$ $ 1.49\times{10}^{46}$
NGC 4548 16.8 $1.83\times{10}^7$   $1.6\times{10}^{-13}$ $2.04\times{10}^{36}$ $ 6.66\times{10}^{44}$
NGC 4565 9.7 $2.15\times{10}^7$   $3.2\times{10}^{-13}$ $1.41\times{10}^{36}$ $ 5.07\times{10}^{44}$
NGC 6500 39.7 $1.15\times{10}^8$   $3.\times{10}^{-14}$ $7.94\times{10}^{38}$ $ 3.08\times{10}^{45}$
FR I            
UGC 00595 181. $2.31\times{10}^8$ 93. $5.8\times{10}^{-18}$ $ 1.82\times{10}^{40}$ $ 5.84\times{10}^{48}$
NGC 0383 67.8 $5.11\times{10}^8$ 92. $1.5\times{10}^{-17}$ $ 2.53\times{10}^{39}$ $ 4.02\times{10}^{48}$
UGC 01841 86.4 $1.78\times{10}^9$ 182. $4.93\times{10}^{-17}$ $ 8.13\times{10}^{39}$ $ 5.85\times{10}^{49 }$
NGC 1218 116. $5.45\times{10}^8$ 964. $2.38\times{10}^{-16}$ $ 7.75\times{10}^{40}$ $ 1.96\times{10}^{50} $
NGC 1275 70.7 $4.4\times{10}^8$ 42 400. $1.5\times{10}^{-15}$ $ 1.27\times{10}^{42}$ $ 3.86\times{10}^{50} $
NGC 3862 82.8 $4.9\times{10}^8$ 200. $1.14\times{10}^{-16}$ $ 8.2\times{10}^{39}$ $ 4.39\times{10}^{49}$
NGC 4261 29.6 $1.19\times{10}^9$ 308. $5.1\times{10}^{-18}$ $ 1.62\times{10}^{39}$ $ 5.16\times{10}^{47}$
NGC 4374 14.8 $8.11\times{10}^8$ 180. $5.9\times{10}^{-17}$ $ 2.36\times{10}^{38}$ $ 1.09\times{10}^{48}$
NGC 4486 14.8 $1.71\times{10}^9$ 4000. $3.9\times{10}^{-16}$ $ 5.24\times{10}^{39}$ $ 1.32\times{10}^{49} $
NGC 5532 95.3 $8.67\times{10}^8$ 77. $3.4\times{10}^{-18}$ $ 4.18\times{10}^{39}$ $ 2.75\times{10}^{48}$
UGC 09799 138. $2.48\times{10}^8$ 391. $9.6\times{10}^{-18}$ $ 4.45\times{10}^{40}$ $ 5.92\times{10}^{48} $
NGC 6166 122. $1.06\times{10}^9$ 105. $1.\times{10}^{-17}$ $ 9.35\times{10}^{39}$ $ 1.56\times{10}^{49}$
NGC 7236 105. $1.22\times{10}^8$ 2. $9.1\times{10}^{-19}$ $ 1.33\times{10}^{38}$ $ 1.85\times{10}^{47}$
UGC 12064 72.7 $4.05\times{10}^8$ 37. $1.8\times{10}^{-17}$ $ 1.17\times{10}^{39}$ $ 4.59\times{10}^{48}$
NGC 7720 121. $1.22\times{10}^9$ 270. $1.9\times{10}^{-17}$ $ 2.37\times{10}^{40}$ $ 3.29\times{10}^{49}$
XBLs            
0158+001 1270. $1.13\times{10}^8$ 11.3 0.047 $1.1\times{10}^{41}$ $ 8.93\times{10}^{50}$
0257+342 1040. $5.36\times{10}^8$ 10. 0.25 $6.49\times{10}^{40}$ $ 1.12\times{10}^{52}$
0317+183 792. $8.12\times{10}^7$ 17. 0.36 $6.39\times{10}^{40}$ $ 2.03\times{10}^{51}$
0419+194 2260. $4.73\times{10}^8$ 8. 0.09 $2.44\times{10}^{41}$ $ 1.71\times{10}^{52}$
0607+710 1130. $5.27\times{10}^8$ 18.2 0.09 $1.39\times{10}^{41}$ $ 4.68\times{10}^{51}$
0737+744 1350. $1.16\times{10}^9$ 24. 0.64 $2.6\times{10}^{41}$ $ 8.92\times{10}^{52}$
0922+745 2860. $7.12\times{10}^9$ 3.3 0.044 $1.62\times{10}^{41}$ $ 1.2\times{10}^{53}$
1207+394 2750. $1.78\times{10}^9$ 5.8 0.1 $2.63\times{10}^{41}$ $ 8.22\times{10}^{52}$
1221+245 914. $8.33\times{10}^7$ 26.4 0.42 $1.32\times{10}^{41}$ $ 3.23\times{10}^{51}$
1229+643 680. $4.17\times{10}^9$ 42. 0.55 $1.16\times{10}^{41}$ $ 5.51\times{10}^{52}$
1407+595 2180. $3.08\times{10}^9$ 16.5 0.07 $4.68\times{10}^{41}$ $ 5.62\times{10}^{52}$
1534+014 1330. $8.01\times{10}^8$ 34. 0.15 $3.61\times{10}^{41}$ $ 1.52\times{10}^{52}$
1757+703 1770. $6.92\times{10}^8$ 7.2 0.18 $1.34\times{10}^{41}$ $ 2.85\times{10}^{52}$
2143+070 998. $3.13\times{10}^8$ 50. 0.32 $2.98\times{10}^{41}$ $ 8.53\times{10}^{51}$
RBLs            
1418+546 629. $1.46\times{10}^9$ 1220. 2.72 $2.89\times{10}^{42}$ $ 1.\times{10}^{53}$
1807+698 206. $2.67\times{10}^{10}$ 1710. 7.85 $4.36\times{10}^{41} $ $ 3.24\times{10}^{53}$
2005-489 289. $1.48\times{10}^9$ 1210. 9.85 $6.03\times{10}^{41}$ $ 7.71\times{10}^{52}$
2200+420 280. $1.71\times{10}^8$ 2140. 8.65 $1.01\times{10}^{42}$ $ 1.12\times{10}^{52}$
2254+074 792. $4.82\times{10}^8$ 560. 0.6 $2.1\times{10}^{42}$ $ 1.43\times{10}^{52}$


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