\begin{table}%t1
%\centering
\par
\caption{Input parameters and results for all simulation runs. Input
  parameters are: electron initial Lorentz factor $\gamma_0$, number density in the beam $n$ in terms of Goldreich-Julian density at the pulsar surface $n_{{\rm GJ}\ast}$, dimensionless
  wiggler strength~$K$, wiggler wavelength $\lambda_{{\rm w}}$,
dimensionless wiggler phase speed $\beta_{{\rm w}}$ and 
  (uniform) background magnetic field~$B_0$. Results from the numerical
  simulations are: central frequency $\nu_{{\rm cen}}$, FWHM
  bandwidth of the radiation $\Delta \nu$, peak power of the light
  pulse~$P_{{\rm max}}$, and brightness temperature corresponding to the
  peak power~$T_{{\rm b}}$. The last four entries are the energy density of
  each ingredient in the simulation: beam $\epsilon_{{\rm b}}$, 
  wiggler $\epsilon_{{\rm w}}$, background magnetic field $\epsilon_{{\rm b0}}$
  and pulse $\epsilon_{{\rm p}}$. Note that every time "-'' appears, it
  means the entry has the value as in run~1. In run~5, {\it n} appears for $\nu_{{\rm res}}$, $\Delta \nu$ and $T_{{\rm b}}$, which means, that for those cases, the spectra are flat, no peaks are seen, and also the brightness temperatures which depend on the bandwidths are not calculated.\label{tabel:inout} }
 % \vspace*{-2mm}
{\begin{tabular}{c|cccccc|cccc|cccc}
\hline\hline
{\bf Run} & \multicolumn{6}{l}{{\bf Input parameters}} & \multicolumn{4}{l}{{\bf Output}} & \multicolumn{4}{l}{{\bf Energy densities}} \\
\hline
 & $\gamma$& $n$ & $K$ & $\lambda_{{\rm w}}$ & $\beta_{{\rm w}}$ & $B_0$ & $\nu_{{\rm cen}}$ & $\Delta \nu$ & $P_{{\rm max}}$ & $T_{{\rm b}}$ & $\epsilon_{{\rm b}}$ & $\epsilon_{{\rm w}}$ & $\epsilon_{{\rm b0}}$ & $\epsilon_{{\rm p}}$ \\
 & & ($n_{{\rm GJ}\ast}$) & & (m) & & (T) & (GHz) & (GHz) & ($10^{13}\:\mbox{W}$) & ($10^{30}\:\mbox{K}$) & ($10^6$ Jm$^{-3}$) & (Jm$^{-3}$) &  (Jm$^{-3}$) &  ($10^2$ Jm$^{-3}$) \\ 
\hline
1 & 1000 & 0.23 & 10 & 50 & 0.9 & 0 & 11 & 2.42 & 9.09 & 1.02 & 1.30 & 8.15 & 0 & 8.25  \\ 
2 & - & - & 5 & - & - & - & 42.8 & 9.72 &36.6 &1.04 &- &2.04 &- &34.5 \\
  & - & - & 10 & - &- &- & 11 &2.42 &9.09 &1.02 &- &8.15 &- &8.25 \\  
  & - & - & 15 & - &- &- &4.96 & 1.02 &3.67 &1.16& - &8.35& - &3.46 \\
  & - & - & 20 & - &- &- &2.84 & 0.53 &1.61 &0.99 &- &32.62& - &1.50 \\
3 & - & - & - & 25 & - & - & 22.2 & 3.8 & 9.52 &  1.44 & - & 32.6 & - & 9.00 \\
& - & - & - & 40 & - & - & 13.8 & 2.86 & 9.42 & 1.02 & - & 10.07 & - & 8.89 \\
& - & - & - &50 & - & - & 11 & 2.42 & 9.09& 1.34&  - & 8.15 & - & 8.25 \\
  & - & - & - & 100 & - & - & 5.57 & 1.28 & 7.02 & 1.70 & - & 2.03 & - & 6.63 \\
4 & - & - & - & - & 0.2 & - & 88.5 & 14.1 & 9.59&  0.215&  - &94.9& -& 9.00 \\
  & - & - & - & - & 0.5 & - & 55.7 & 8.12 & 9.54 & 0.37 & - & 18.2 & - & 9.00 \\
  & - & - & - & - & 0.8 & - & 22.2 & 3.79 &9.39 &0.79 &- &9.35 &- &8.86 \\
  & - & - & - & - & 0.9 & - & 11 & 2.42 &9.09 &1.02 &- &8.15 &- &8.25 \\
5 & - & - & - & - & - & $10^{-3}$ & 10.9 & 2.43& 9.46 &7.4 &- &- &0.4 &8.85 \\
  & - & - & - & - & - & $0.01$ & 2.18 & 0.61 &2.7 &1.36 &- &- &40 &2.55 \\
  & - & - & - & - & - & $0.025$ & n & n & 0.455 & n & - & - & $2.48 \times 10^2$& $42.8 \times 10^{-2}$\\ 
  & - & - & - & - & - & $0.05$ & n & n & $6.36 \times 10^{-4}$ & n & - & -& $9.95 \times 10^{2}$ & $4.0 \times 10^{-4}$ \\ 
%  & - & - & - & - & - & $0.075$ & n & n & $4.29 \cdot 10^{-5}$ & n & - & -& $2.24\times 10^3$ & $4.05 \times 10^{-5}$ \\ 
%  & - & - & - & - & - & $0.1$ & n & n & $8.31 \cdot 10^{-6}$ & n & - & -& $3.98\times  10^3$ & $7.84 \times 10^{-6}$\\ 
6  & - & $0.1$ & - & - & - & - & 11.37 & 1.53 & 1.79 & 0.38 & 2.30 & -& -& $1.7$\\ 
  & - & $0.2$ & - & - & - & - & 11.1 & 2.22 & 7.2 & 1.07 & 1.76 & - & - & $6.8$\\ 
  & - & $0.3$ & - & - & - & - & 10.9 & 3.01& 16.5 & 1.73 & 1.15 & - & - & $15.5$\\ 
  & - & $0.4$ & - & - & - & - & 10.7 & 3.40 & 29.9 & 2.8 &0.575& - &- & $28.2$ \\ 
7 & 1000 & -  & - & - & - & - & 11 & 2.42 &9.09 &1.24 & 1.3 &- &- &8.24 \\
  & 500 & -  & - & - & - & - & 2.72 &0.80 &1.77 &0.72 &0.16 &- &- &1.66 \\
  & 250 & -  & - & - & - & - & 0.69 &0.16 &0.112 &0.23& 0.02 &- &-&0.10 \\
  & 100 & -  & - & - & - & - & 0.09 & 0.006 & $2.7\times 10^{-4}$ &$4.6\times 10^{-3}$ & $1.36\times 10^{-3}$&- & - & $2.5 \times 10^{-4}$ \\
\hline 
\end{tabular}}
\end{table}