\begin{table}%t4
\caption{\label{eroseventtable}The 11  events of the EROS collaboration used in the past to set upper
limits on the microlensing optical depth toward
the LMC~and to measure the depth toward the 
SMC.  
Candidates marked "B-S'' in Col.~2 occur on stars in the EROS-2 
Bright-Star Sample.
All candidates except EROS2-SMC-1 
have been eliminated as variable stars or as supernovae.
}
\small%\centering
\par
 \begin{tabular}{l l l l l l } 
 \hline\hline
Candidate & EROS-2 star     & $\reros$ & $(B-R)_{\rm eros}$ & Original ref.  & Status  \\
\hline
EROS1-LMC-1     & lm058-2k-21915    &   18.75 &    0.34 & \citet{aub93} & $2${nd} variation  \citep{tis04} (Figure \ref{eros1-1fig})       \\
EROS1-LMC-2     & lm043-6m- 9377 B-S  &   19.32 &   --0.04 & \citet{aub93} & $2${nd} variation    \citep{las00}       \\
EROS2-LMC-3 & lm034-6l-20493    &   20.90 &    0.61 & \citet{las00} &  $2${nd} variation   \citep{tis04}       \\
EROS2-LMC-4 & lm018-6n-23236    &   19.10 &    1.87 & \citet{las00} &   $2${nd} variation  \citep{mil00}       \\
EROS2-LMC-5 & lm015-3n-22431 B-S  &   19.17 &    0.14 & \citet{mil00} &  Supernova  \citep{tis04}                 \\
EROS2-LMC-6 & lm067-5m-14700    &   21.01 &    0.63 & \citet{mil00} &  Supernova  \citep{tis04}                 \\
EROS2-LMC-7 & lm070-3n-23389    &   21.00 &    0.76 & \citet{mil00} &  Supernova  \citep{tis04}                 \\
EROS2-SMC-1 & sm005-4m-5761 B-S  &   18.13 &   --0.13 & Palanque-D. et~al. (1998)&  Fig.~\ref{smc1fig}                      \\
EROS2-SMC-2 & sm001-6l-13221 B-S  &   19.56 &    0.44 & \citet{EROSMC}&  long period variable \citep{tis04}       \\
EROS2-SMC-3 & sm001-6n-16904 B-S  &   19.31 &    0.59 & \citet{EROSMC}&  long period variable \citep{tis04}       \\
EROS2-SMC-4 & sm002-7m-21331 B-S  &   19.48 &    0.32 & \citet{EROSMC}&  long period variable \citep{tis04}       \\
\hline
\end{tabular}
\end{table}