\begin{table}%tB.1 \caption{\label{tab:fulltable}Full sample from Papers~I, II and present paper, used in the correlation fits.} %\centerline { \begin{tabular}{lcccrcccr} \hline\hline Source & Type & Distance & $r_0$ & Filter & \multicolumn{1}{c}{Flux} & \multicolumn{1}{c}{$\log$~\lmir} & \multicolumn{1}{c}{$\log$~\lx} & \alphaix\\ & & Mpc & pc & & \multicolumn{1}{c}{mJy} & \multicolumn{1}{c}{erg s$^{-1}$} & \multicolumn{1}{c}{erg s$^{-1}$} & \\ (1)& (2) & (3) & (4) & (5) & \multicolumn{1}{c}{(6)} & \multicolumn{1}{c}{(7)} & \multicolumn{1}{c}{(8)} & (9) \\ \hline%_____________________________________________________________________________________________________________ \object{Fairall 9}& 1.2 & 206 & 320 & NEII & 306 $\pm$ 10 & 44.51 $\pm$ 0.03 & 43.87 $\pm$ 0.15 & --1.21\\ \object{NGC 526A}& 1.9 & 81 & 135 & NEII\_1 & 275 $\pm$ 55 & 43.70 $\pm$ 0.08 & 43.14 $\pm$ 0.10 & --1.21\\ \object{SWIFT J0138.6-4001}& 2 & 108 & 175 & PAH2 & 34 $\pm$ 3 & 43.10 $\pm$ 0.04 & 43.59 $\pm$ 0.30 & --0.96\\ \object{Mrk 590}& 1 & 112 & 175 & NEII & 106 $\pm$ 13 & 43.55 $\pm$ 0.06 & 43.61 $\pm$ 0.25 & --1.06\\ \object{NGC 1068}& CT & 14 & 25 & * &9500 $\pm$ 475 & 43.80 $\pm$ 0.03 & 43.40 $\pm$ 0.30 & --1.16\\ \object{NGC 1097}& L & 17 & 30 & NEII\_1 & 28 $\pm$ 7 & 41.40 $\pm$ 0.11 & 40.80 $\pm$ 0.15 & --1.22\\ \object{SWIFT J0601.9-8636}& 2 & 25 & 45 & NEII\_2 & 72 $\pm$ 15 & 42.11 $\pm$ 0.08 & 41.92 $\pm$ 0.30 & --1.10\\ \object{ESO 209-G012}& 1.5 & 179 & 280 & NEII & 188 $\pm$ 26 & 44.22 $\pm$ 0.06 & 43.65 $\pm$ 0.15 & --1.21\\ \object{NGC 3081}& 1h & 34 & 55 & NEII\_2 & 138 $\pm$ 11 & 42.64 $\pm$ 0.04 & 42.60 $\pm$ 0.30 & --1.07\\ \object{ESO 263-G013}& 2 & 143 & 225 & NEII & 46 $\pm$ 3 & 43.42 $\pm$ 0.02 & 43.30 $\pm$ 0.40 & --1.09\\ \object{NGC 3281}& CT & 46 & 75 & NEII\_2 &1016 $\pm$ 52 & 43.76 $\pm$ 0.02 & 43.30 $\pm$ 0.15 & --1.16\\ \object{NGC 3393}& CT & 53 & 90 & NEII\_2 & 94 $\pm$ 5 & 42.90 $\pm$ 0.02 & 43.04 $\pm$ 0.30 & --1.01\\ \object{NGC 3783}& 1.5 & 43 & 70 & NEII\_1 & 722 $\pm$ 67 & 43.52 $\pm$ 0.05 & 43.21 $\pm$ 0.15 & --1.15\\ \object{NGC 4388}& 1h & 17 & 30 & NEII\_2 & 375 $\pm$ 28 & 42.45 $\pm$ 0.03 & 42.24 $\pm$ 0.30 & --1.11\\ \object{NGC 4507}& 1h & 51 & 80 & NEII\_1 & 685 $\pm$ 50 & 43.67 $\pm$ 0.04 & 43.30 $\pm$ 0.15 & --1.17\\ \object{NGC 4579}& L & 21 & 35 & NEII\_1 & 61 $\pm$ 21 & 41.88 $\pm$ 0.14 & 41.10 $\pm$ 0.15 & --1.26\\ \object{NGC 4593}& 1 & 38 & 65 & NEII\_1 & 382 $\pm$ 73 & 43.18 $\pm$ 0.08 & 42.93 $\pm$ 0.20 & --1.13\\ \object{IC 3639}& CT & 46 & 75 & NEII\_2 & 542 $\pm$ 29 & 43.51 $\pm$ 0.02 & 43.62 $\pm$ 0.50 & --1.04\\ \object{ESO 323-G032}& 1.9 & 68 & 110 & PAH2 & 61 $\pm$ 6 & 42.96 $\pm$ 0.04 & 42.43 $\pm$ 0.40 & --1.24\\ \object{NGC 4941}& 2 & 17 & 30 & NEII\_1 & 81 $\pm$ 6 & 41.74 $\pm$ 0.05 & 41.30 $\pm$ 0.30 & --1.18\\ \object{NGC 4992}& 2 & 108 & 175 & NEII & 71 $\pm$ 4 & 43.36 $\pm$ 0.02 & 43.23 $\pm$ 0.30 & --1.09\\ \object{IRAS 13197-1627}& 1h & 73 & 115 & NEII\_1 & 875 $\pm$ 46 & 44.07 $\pm$ 0.03 & 42.78 $\pm$ 0.20 & --1.31\\ \object{Cen A}& 2 & 3.8 & 7 & NEII\_1 &1451 $\pm$ 73 & 41.80 $\pm$ 0.04 & 41.68 $\pm$ 0.15 & --1.10\\ \object{NGC 5135}& CT & 60 & 95 & NEII\_1 & 123 $\pm$ 12 & 43.06 $\pm$ 0.05 & 43.00 $\pm$ 0.50 & --1.07\\ \object{MCG-06-30-15}& 1.5 & 34 & 55 & NEII\_1 & 393 $\pm$ 49 & 43.07 $\pm$ 0.06 & 42.74 $\pm$ 0.20 & --1.10\\ \object{NGC 5728}& CT & 38 & 65 & NEII\_2 & 123 $\pm$ 10 & 42.69 $\pm$ 0.03 & 42.80 $\pm$ 0.30 & --1.03\\ \object{NGC 5995}& 2 & 108 & 170 & NEII & 421 $\pm$ 61 & 44.11 $\pm$ 0.06 & 43.54 $\pm$ 0.15 & --1.20\\ \object{ESO 138-G001}& CT & 38 & 65 & NEII\_2 & 862 $\pm$ 45 & 43.54 $\pm$ 0.02 & 43.00 $\pm$ 0.30 & --1.17\\ \object{NGC 6300}& 2 & 16 & 25 & NEII\_2 & 727 $\pm$ 38 & 42.69 $\pm$ 0.02 & 42.30 $\pm$ 0.30 & --1.11\\ \object{ESO 103-G035}& 2 & 57 & 95 & NEII\_2 & 622 $\pm$ 49 & 43.74 $\pm$ 0.03 & 43.44 $\pm$ 0.15 & --1.14\\ \object{ESO 141-G055}& 1 & 156 & 240 & NEII\_1 & 170 $\pm$ 47 & 44.04 $\pm$ 0.11 & 43.90 $\pm$ 0.15 & --1.10\\ \object{NGC 6814}& 1.5 & 21 & 35 & NEII\_2 & 96 $\pm$ 6 & 42.07 $\pm$ 0.02 & 42.12 $\pm$ 0.40 & --1.07\\ \object{Mrk 509}& 1.5 & 147 & 225 & NEII & 269 $\pm$ 42 & 44.18 $\pm$ 0.07 & 44.10 $\pm$ 0.15 & --1.11\\ \object{PKS 2048-57}& 1h & 47 & 80 & NEII\_1 &1035 $\pm$ 108 & 43.82 $\pm$ 0.05 & 42.84 $\pm$ 0.20 & --1.30\\ \object{PG 2130+099}& 1.5 & 274 & 415 & NEII & 179 $\pm$ 31 & 44.53 $\pm$ 0.07 & 43.65 $\pm$ 0.20 & --1.24\\ \object{NGC 7172}& 2 & 38 & 60 & NEII\_1 & 165 $\pm$ 27 & 42.79 $\pm$ 0.07 & 42.76 $\pm$ 0.40 & --1.09\\ \object{NGC 7213}& L & 25 & 40 & NEII\_1 & 271 $\pm$ 27 & 42.67 $\pm$ 0.05 & 42.23 $\pm$ 0.15 & --1.18\\ \object{3C 445}& 1.5 & 247 & 365 & NEII & 206 $\pm$ 28 & 44.50 $\pm$ 0.06 & 44.26 $\pm$ 0.15 & --1.16\\ \object{NGC 7314}& 1h & 21 & 35 & PAH2 & 75 $\pm$ 22 & 41.96 $\pm$ 0.12 & 42.20 $\pm$ 0.15 & --1.01\\ \object{NGC 7469}& 1.5 & 68 & 110 & NEII\_1 & 627 $\pm$ 35 & 43.92 $\pm$ 0.03 & 43.15 $\pm$ 0.10 & --1.24\\ \object{NGC 7674}& CT & 125 & 195 & NEII & 506 $\pm$ 29 & 44.31 $\pm$ 0.03 & 44.56 $\pm$ 0.50 & --1.00\\ \object{NGC 7679}& 2 & 73 & 115 & NEII\_1 & 46 $\pm$ 18 & 42.82 $\pm$ 0.15 & 42.52 $\pm$ 0.15 & --1.14\\ \hline \end{tabular}} \par \medskip Targets listed in order of increasing right ascension. In Col. (2), L = LINER and CT = Compton-thick. Column (4) lists approximate physical scale corresponding to an angular resolution limit of 0\farcs35. * For NGC 1068, observations around 12~\micron\ from Tomono et~al. (2001) and Mason et~al. (2006) were used. Refer to Table~\ref{tab:fluxes} and the text for other details. \end{table}