\begin{table}%t1
%\centering
\par
\caption{\label{tab:standardsummary}Parameter values of our standard
  scenario.}
  \begin{tabular}[h]{l@{\hspace{-1mm}}r l p{4.3cm}}
    \hline\hline\noalign{\smallskip}
    & Parameter & Standard value & Comment\\
    \hline
    &$D_{\rm S}$ & $8$~kpc & distance to Galactic bulge  \\
    &$D_{\rm L}$ & $6$~kpc &   \\
    &$M_{\rm Star}$ & $0.3~M\ensuremath{_{\sun}}$ & most abundant
    type of star  \\ 
    &$\mu_\perp$ & $7~{\rm mas/year}$ & ${=}v_\perp=200$~km~s$^{-1}$
    at $D_{\rm L}=6$~kpc  \\
    *&$q_{\rm PS}$ & $10^{-3}$ &  Jupiter/Sun mass ratio\\
    *&$\theta_{\rm PS}$ & $1.3~\ensuremath{\theta_{E}}$ &  wide
    separation caustic \\ 
    *&$q_{\rm MP}$ & $10^{-2}$ & Moon/Earth mass ratio \\
    *&$\theta_{\rm MP}$ & $1.0~\ensuremath{\theta_{E}}^P$ &
    planetary Einstein radius\\ 
    *&$R_{\rm Source}$ & $R_{\sun}$ & brightness requirements
    vs. stellar abundance \\ 
    *&$f_{\rm sampled}$ & $\simeq\frac{1  ~{\rm frame}}{15~{\rm min}}$ &  high-cadence observation \\ 
    *&$\sigma$ & 20~mmag & typical value in past observations \\
    \hline
  \end{tabular}
\tablefoot{Parameters marked with an asterisk~(*) are varied in our
  simulations in order to evaluate their influence on the lunar detection
  rate and to compare different triple-lens scenarios. The fixed
  parameters lead to values for the Einstein ring radius,
  $\ensuremath{\theta_{E}} =0.32$~mas, i.e.~1.9~AU
    in the lens plane, and the Einstein
  time, $t_E \simeq 17$~days. 
    The lensed system is a Saturn-mass planet at a projected
  separation of 2.5~AU from its $0.3~M_{\sun}$ M-dwarf
  host, the Earth-mass satellite orbits the planet at 0.06~AU,
  i.e.~$0.01$~mas angular separation, cf. Fig.~\ref{fig:lensingzones}.}
\vspace*{-2mm}
\end{table}