\begin{table}%t1
%\centering
\par
\caption{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 
\protect\citet{MerrittFerrarese2001}. 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.~(\ref{scaledX-rays}). This luminosity has also
been corrected for the different observed energy bands assuming a
photon index of~1.6.\label{tableAGN}}
\begin{tabular}{p{0.12\linewidth}cccccc}
\hline\hline
 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] $& $\left[\mbox{erg}/ \mbox{s}\right]$\\
             \hline
 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}$ \\
\hline 
 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}$ \\
\hline 
 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}$
 \\
\hline 
 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}$ \\
\hline 
 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}$ \\
           \hline
          \end{tabular}
\end{table}