\begin{table}%t2
\caption{Exemplary flare distribution properties for the black hole/disk system
seen at a moderate inclination, $i=30{\degr}$. 
Parameters above the double line are assumed while the parameters below the 
double line are calculated as described in Sect.~\ref{sect:flares}.
\label{tab:properties}}
%\centerline
$$
{\begin{tabular}{llcrrrrrrrrrrrrr}  
\hline\hline
&\multicolumn{1}{c}{\hspace*{-2ex}Parameter} & & \multicolumn{13}{c}{Model\rule[-2ex]{0mm}{5ex}}\\
&                & & A      & B       & C      & D      & E      & F      & G      & I      & J      & K     & L    &  P   &  Q\\
\cline{1-2}\cline{4-16}
\rule{0mm}{4ex}
&$M$             & &$10^8$  &$10^8$   &$10^8$  &$10^8$  &$10^8$  &$10^8$  &$10^8$  &$10^8$  &$10^8$  &$10^8$ &$10^7$&$10^7$&$10^7$\\  
&$R_{\rm{}in}$        & & 6      & 6       &  6     & 1.2    & 6      & 6      & 6      & 6      & 6      & 6     & 1.2  & 1.2  & 1.2\\
&$R_{\rm{}out}$       & & 50     & 50      &  50    & 50     & 100    & 50     & 50     & 50     & 50     & 50    & 50   & 50   & 50\\
&$\beta_{\rm{}rad}$   & & 3      & 3       &  3     & 3      & 3      & 2.5    & 3      & 3      & 4      & 3     & 3    & 3    & 3\\
&$L_{\rm{}X}$         & & 1      & 1       &  1     & 1      & 1      & 1      & 1      & 1      & 1      & 0.1   & 0.5  & 0.5  & 0.5\\
\begin{rotate}{90}Assumed\end{rotate}
&$n_{\rm{}mean}$      & & 30     & 30      & 10     & 100    & 30     & 100    & 30     & 100    & 100    & 30    & 3000 & 1000 & 300\\
&$t_{\rm{}life}$      & & $10^5$ & $10^3$  & $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^5$&$10^5$&$10^5$&$10^5$\\
&$T_{\rm{}obs}$       & & $10^5$ &  $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^5$ & $10^4$ & $10^5$ & $10^5$ & $10^5$&$10^3$&$10^3$&$10^3$\\
\hline 
\rule{0mm}{4ex}
&$R_{\rm{}X}^{\rm{}a}$   & & 2.65   & 2.65    & 4.59   & 0.62   & 5.16   & 1.57   & 2.65   & 1.45   & 1.16   & 0.84 & 0.24  & 0.43 & 0.80\\
&$R_{\rm{}X}^{\rm{}b}$   & & 3.17   & 3.17    & 6.11   & 0.79   & 7.42   & 1.67   & 3.17   & 1.68   & 1.32   & 0.89 & 0.28  & 0.52 & 1.10\\
&$N_{\rm{}mean}$         & & 60     & 3030    & 20     &200     & 60     & 200    & 33     & 200    & 200    & 60   & 3030  & 1010 & 300\\
&$c_{\rm{}mean}$         & & 0.12   & 0.12    & 0.15   &0.025   & 0.16   & 0.11   & 0.12   & 0.10   & 0.07   & 0.010& 0.09  & 0.11 & 0.14\\
&$F_{\rm{}var}^{\rm{}a}$ & & 43     & 6.0     & 74     &107     & 81     & 18     & 58     & 24     & 34     & 43   & 27    & 47   & 87\\
\begin{rotate}{90}Determined\end{rotate}
&$F_{\rm{}var}^{\rm{}b}$ & & 28     & 4.0     & 38     &64      & 36     & 15     & 38     & 19     & 26     & 37   & 22    & 33   & 45\\
&$F_{\rm{}var}$& & 26       &  3.8       & 39      &27      & 36       & 13       & 36       & 17       & 25       & 32   & 7.0      &  15    &  28 \\
\hline     
\end{tabular}}
$$
\smallskip
$M$ is the black hole mass in $M_{\odot}$; $R_{\rm{}in}$, $R_{\rm{}out}$ and 
$R_{\rm{}X}^{\cdots}$ 
are the disk and the spot characteristic radii in $R_{\rm{}g}=GM/c^2$
(radius $R_{\rm{}X}^{\rm{}a}$ of the spot orbit follows from 
Eq.~(\ref{eq:RX}), while
$R_{\rm{}X}^{\rm{}b}$ includes correction on finite size of spots);
luminosity $L_{\rm{}X}$ is in units of $10^{44}$~erg~s$^{-1}$~cm$^{-2}$; time intervals $t_{\rm{}life}$, $T_{\rm{}obs}$ are 
in seconds; variances $F_{\rm{}var}^{\cdots}$ are in percent; 
($F_{\rm{}var}^{\rm{}a}$ follows from Eq.~(\ref{eq:Nvar}), 
$F_{\rm{}var}^{\rm{}b}$ includes
the effect of the spot finite size and 
$F_{\rm{}var}^{\rm{}}$ was obtained numerically at 1~keV with 
relativistic corrections and finite size of the spots taken into account).
\end{table}