\begin{table}%t1     
\caption{\label{tab1}Two-peak MQ vs Pulsar Model.}     
\par
%\centerline
{ \small
\begin{tabular}{c c c c}     
\hline\hline       
&PSR B1259-63 & Two-peak Microquasar & \lsi \\ 
\hline                    
radiopulses & yes & no & no\\  
$L_{\rm X}$ [erg/s] & $5 \times 10^{34}$\tablefootmark{a}& $10^{33.5}{-}10^{36}$\tablefootmark{b}  & $(1{-}6) \times 10^{34}$\tablefootmark{c}\\
Largest radio outburst& toward periastron\tablefootmark{d} & toward apastron\tablefootmark{e} & toward apastron\tablefootmark{f} \\
Radio spectral index& $\alpha < 0$\tablefootmark{d}& $\alpha\ge 0$  then  $\alpha < 0$\tablefootmark{g}&  $\alpha \geq 0$ then  $\alpha < 0$  twice per orbit\tablefootmark{b}\\
Gamma-ray peak& toward periastron\tablefootmark{h}&  EIC at periastron, dominant SSC toward apastron\tablefootmark{e,~i}
& Two peaks: EGRET/VERITAS/FERMI\tablefootmark{i}\\
\hline                  
\end{tabular}}
\tablefoot{\tablefoottext{a}{Kaspi et~al. 1995.} 
\tablefoottext{b}{Massi \& Kaufman Bernad{\'o} \cite{Massi2009}.} 
\tablefoottext{c}{Paredes et~al. 1997.} 
\tablefoottext{d}{Connors et~al. \cite{Connors2002}.}  
\tablefoottext{e}{Bosh-Ramon 2006.} 
\tablefoottext{f}{Fig.~\ref{fig2}-c in Massi \& Kaufman Bernad{\'o} \cite{Massi2009}.} 
\tablefoottext{g}{Fender et~al. \cite{Fender2004}.} 
\tablefoottext{h}{Aharonian et~al. \cite{Aharonian2009}.} 
\tablefoottext{i}{see Sect.~1.}}    
\end{table}