\begin{table}%t2
\caption {\label{Tab:artstat}Results of Monte Carlo modeling of
  background plus one star (100~tries) as shown in
  Fig.~\ref{Fig:artim}.}
%\centerline
 {\begin{tabular}[htb]{llllllllll}
\hline\hline
 & $x^{{a}}$ & $\sigma_{x,\rm formal}^{{b}}$ & $\sigma_{x,\rm true}^{{c}}$  & $y^{{d}}$ & $\sigma_{y,\rm formal}^{{\rm e}}$ & $\sigma_{y,\rm true}^{{f}}$ & $f^{{g}}$ & 
 $\sigma_{f,\rm formal}^{{h}}$ & $\sigma_{f,\rm true}^{{i}}$ \\
 & [pix] & [pix] & [pix] & [pix] & [pix] & [pix] & [counts] & [counts]  & [counts]\\
\hline
raw & 75.670 & 0.009 & 0.009 & 75.109 & 0.008 & 0.009 & 1000 & 4 &4\\
deconvolved & 75.670 & 0.003 & 0.011 & 75.108 & 0.003 & 0.010 & 1000& 2 & 7 \\
\hline
\end{tabular}}
\par
\smallskip
$^{{a}}$ Measured position of the star on the $X$-axis (model position $x=75.670$)
$^{{b}}$ $1\sigma$ uncertainty of  measured $x$ given by the PSF fitting algorithm (average of the uncertainties of all the tries)
$^{{c}}$ $1\sigma$ uncertainty of measured $x$ as given by the standard deviation of the individual measurements
$^{{d}}$~Measured position of the star on the $Y$-axis (model position $x=75.110$)
$^{{e}}$ $1\sigma$ uncertainty of measured $y$ given by the PSF fitting algorithm (average of the uncertainties of all the tries)
$^{{f}}$ $1\sigma$ uncertainty of measured $y$ as given by the standard deviation of the individual measurements
$^{{g}}$~Measured flux of the star (input flux $f=1000.0$)
$^{{h}}$ $1\sigma$ uncertainty of measured $f$ given by the PSF fitting algorithm (average of the uncertainties of all the tries)
$^{{i}}$ $1\sigma$ uncertainty of measured $f$ as given by the standard deviation of the individual measurements.
\end{table}