\begin{table}%t1
\caption{\label{tab1}Variable stars in the MACHO field \#1.}
\par
\small%\centerline
 {
\begin{tabular}{ccclrrc}
\hline\hline
%&&&&&& \\[-8pt]
 ID  &  $V$  & $V-R$  &  $f$[d$^{-1}$] &  {\it SNR}  &  Type  & TFA \\
\hline
05011976$-$6921083 & 16.889 &  0.101 &  1.80367  &  14.5 & B       & 1\\
05011992$-$6919188 & 17.585 &  0.049 &  0.37573  &  10.8 & B       & 0\\
05011998$-$6917495 & 18.066 &  0.430 &  0.252205 &  16.9 & EB      & 0\\
05012021$-$6920315 & 18.940 &  0.582 &  7.82853  &   7.0 & d Sct?  & 1\\
05012029$-$6920248 & 19.615 &  0.113 &  0.02328  &  13.9 & LPV     & 0\\
\hline
\end{tabular}}                                                         
\medskip                                                      
{Notes:}
\par
$-$ The object identification follows the notation of the 2MASS catalog, namely it is simply the abbreviated J2000 (RA,~Dec)~coordinates of the object. For example, 05011976$-$6921083 corresponds to RA~= 05:01:19.76, Dec~= $-$69:21:08.3.  
\par
$-$ The frequencies for type EB variables are given by a larger number of digits, because of the higher sensitivity of the eclipse shape to the precision of the orbital period.
\par
$-$ The definition of the signal-to-noise ratio ({\it SNR}) and classification scheme are described in the text.
\par
$-$ Single digits under the column ``TFA'' mean exclusive TFA detections if~``1'' and pre-TFA detections if~``0''.    
\par
$-$ The excerpt shown is part of the full table, which is only available at the CDS.%in the electronic version of this paper.
\end{table}