\begin{table}%t2
%\centering
\par
\caption{Best fit results for the KFC sample and the original and edited MHDM sample. Besides the full sample we also give the parameters for the subsamples containing only a limited set of AGN classes. Note that LINER sources classified by MHDM are not limited to LLAGN. The LH~XRB sample is defined in Sect.~\ref{secsample}. The column~$N$ denotes the number of sources in the sample.\label{tabresult}
 } 
\begin{tabular}{lccccccc}
\hline \hline
\noalign{\smallskip}
&  $\xi_{\rm R}$ & $\xi_{\rm M}$ & $b_{\rm X}$& $\sigma_{\rm int}$ &$\xi_{\rm m}|\xi{r} = 1.4$ & $\sigma_{\rm int}|\xi{r} = 1.4$ & $N$ \\
\hline \noalign{\smallskip}
\multicolumn{2}{l}{KFC sample}\\
\noalign{\smallskip}
Full sample & $1.41 \pm 0.11$ & $-0.87 \pm 0.14$ & $-5.01 \pm 3.20$ & 0.38 & $-0.86 \pm 0.02$ & 0.38 & 77\\
(XRB, Sgr A$^*$, LLAGN, FR-I, BL Lac) \\
\noalign{\smallskip}Full sample + Seyferts \& Transition obj. & $1.48 \pm 0.13$ & $-0.95 \pm 0.16$ & $-6.89 \pm 3.83$ & 0.44 & $-0.86 \pm 0.02$ & 0.44 & 100\\
\noalign{\smallskip}XRB, Sgr A$^*$, LLAGN, FR-I& $1.25 \pm 0.10$ & $-0.74 \pm 0.12$ & $-0.46 \pm 2.93$ & 0.28 & $-0.91 \pm 0.02$ & 0.30 & 58\\
\noalign{\smallskip}XRB, Sgr A$^*$, LLAGN, BL Lac, & $1.64 \pm 0.13$ & $-1.08 \pm 0.14$ & $-11.67 \pm 3.59$ & 0.18 & $-0.81 \pm 0.02$ & 0.23 & 62\\
\noalign{\smallskip}XRB, Sgr A$^*$, LLAGN & $1.59 \pm 0.21$ & $-1.02 \pm 0.21$ & $-10.15 \pm 6.17$ & 0.12 & $-0.84 \pm 0.02$ & 0.15 & 43\\
\noalign{\smallskip}XRB, Sgr A$^*$, LLAGN, Seyfert \& Transition &  $1.86 \pm 0.35$ & $-1.33 \pm 0.36$ & $-17.98 \pm 9.92$ & 0.35 & $-0.85 \pm 0.02$ & 0.39 & 66\\
\noalign{\smallskip}Sgr A$^*$, LLAGN, FR-I, BL Lac &  $1.70 \pm 1.17$ & $-2.17 \pm 4.09$ & $-5.21 \pm 12.08$ & 0.45 & $-1.15 \pm 0.38$ & 0.46 & 52\\
\noalign{\smallskip}\hline\noalign{\smallskip}
\noalign{\smallskip} Full sample with quiescent Sgr A$^*$ &  $1.52 \pm 0.14$ & $-1.00 \pm 0.18$ & $-8.15 \pm 4.11$ & 0.39 & $-0.85 \pm 0.02$ & 0.40 & 77 \\
\noalign{\smallskip}XRB, quiescent Sgr A$^*$, LLAGN & $1.97 \pm 0.11$ & $-1.41 \pm 0.10$ & $-21.05 \pm 3.05$ & 0.00 & $-0.86 \pm 0.02$ & 0.23 & 43\\
\noalign{\smallskip}\hline\noalign{\smallskip}
Original MHDM sample &$1.45 \pm 0.17$ & $-0.99 \pm 0.22$ & $-5.98 \pm 5.02$ & 0.72 & $-0.93 \pm 0.03$ & 0.73 & 116\\  
\noalign{\smallskip}\hline \noalign{\smallskip}
\multicolumn{3}{l}{MHDM sample with LH XRBs}\\
 \noalign{\smallskip}
Full sample & $1.74 \pm 0.20$ & $-1.35 \pm 0.27$ & $-14.23 \pm 5.75$ & 0.65 & $-0.92 \pm 0.03$ & 0.68 & 103\\
(XRB, Sgr A$^*$, LINER, Quasar, Seyfert) \\
\noalign{\smallskip}XRB, Sgr A$^*$, LINER, Seyfert &  $1.55 \pm 0.19$ & $-1.15 \pm 0.24$ & $-8.93 \pm 5.37$ & 0.64 & $-0.96 \pm 0.03$ & 0.64 & 92\\
\noalign{\smallskip}XRB, Sgr A$^*$, LINER, Quasar &  $2.12 \pm 0.31$ & $-1.75 \pm 0.38$ & $-25.20 \pm 8.81$ & 0.51 & $-0.90 \pm 0.04$ & 0.62 & 57\\
\noalign{\smallskip}XRB, Sgr A$^*$, Quasar, Seyfert&  $1.79 \pm 0.28$ & $-1.39 \pm 0.37$ & $-15.68 \pm 7.87$ & 0.63 & $-0.88 \pm 0.03$ & 0.65 & 82\\
\noalign{\smallskip}XRB, Sgr A$^*$, LINER &  $1.59 \pm 0.35$ & $-1.19 \pm 0.40$ & $-10.11 \pm 10.13$ & 0.50 & $-1.54 \pm 0.21$ & 0.71 & 46\\
\noalign{\smallskip}XRB, Sgr A$^*$, Quasar &  $2.03 \pm 0.28$ & $-1.55 \pm 0.36$ & $-22.76 \pm 7.86$ & 0.14 & $-0.74 \pm 0.04$ & 0.32 & 37\\
\noalign{\smallskip}Sgr A$^*$, LINER, Quasar, Seyfert & $1.65 \pm 0.26$ & $-1.72 \pm 0.50$ & $-8.02 \pm 8.06$ & 0.74 & $-1.41 \pm 0.22$ & 0.76 & 78\\
\hline
\end{tabular}
\end{table}