\begin{table}%T2
%\centering
\par
\caption{Name, spectral type, amplitude of the light curve,
photometric and orbital periods and interstellar extinction correction
for the stars lying below the "zero excess'' line in Fig.~\ref{excess}.}
\label{extinct}
\begin{tabular}{rrllccccc}
\hline 
\hline 
\multicolumn{1}{c}{CABS}  & \multicolumn{1}{c}{HD} & 
\multicolumn{1}{c}{Other} & Sp.Ty. & \multicolumn{1}{c}{$\Delta V$} &
\multicolumn{1}{c}{$P_{\rm{ph}}$} & \multicolumn{1}{c}{$P_{\rm{orb}}$}
& $E(U-B)$ & $E(B-V)$ \\
& & & & \multicolumn{1}{c}{(mags.)} & \multicolumn{1}{c}{(days)} &
\multicolumn{1}{c}{(days)} & & \\
\hline
78  & 72688  & VX Pyx    & K0~III  & 0.04 & 19.34 & 45.130 & 0.184 & 0.255 \\
85  & 81410  & IL Hya    & K1~III  & 0.45 & 12.89 & 12.908 & 0.090 & 0.130 \\
86  & 83442  & IN Vel    & K2~IIIp & 0.30 & 54.95 & 52.270 & 0.360 & 0.500 \\
165 & 181809 & V4138 Sgr & K1~III  & 0.35 & 60.23 & 13.048 & 0.110 & 0.160 \\
\hline
\end{tabular}
\end{table}