\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}