\begin{table}%t2
\caption{Pulsation parameters ($T_0$ is the Julian date of the reference epoch,
$P$ is the period in days)
and color excesses (from Fernie \cite{fernie90}) for the Cepheids discussed in this paper.
$(B-V)_0$ is the mean dereddened $(B-V)$~color as reported in the online database by
Fernie et~al. (\cite{fernie95}).}
\label{cepheid_mag_extinct}
%\centering
\par
\begin{tabular}{lcccc}
\hline \hline
Star & $T_0$ (JD) & $P$ (days) & $(B-V)_0$ & $E(B-V)$ \\
\hline
$\alpha$~UMi & 2~439~253.230 & 3.972676 & 0.598 & --0.007  \\
$\delta$~Cep & 2~436~075.445 & 5.366341 & 0.657 & 0.092 \\
X~Sgr & 2~452~723.949 & 7.013059 & 0.739 & 0.197 \\
$\eta$~Aql & 2~445~342.479 & 7.176769 & 0.789 & 0.149 \\
W~Sgr & 2~452~519.248 & 7.594904 & 0.746 & 0.111 \\
$\beta$~Dor & 2~452~214.215 & 9.842425 & 0.807 & 0.044 \\
$\zeta$~Gem & 2~442~059.774 & 10.15097 & 0.798 & 0.018 \\
Y~Oph & 2~452~715.481 & 17.12691 & 1.377 & 0.655 \\
$\ell$~Car & 2~452~290.416 & 35.55134 & 1.299 & 0.170 \\
\hline
\end{tabular}
\end{table}