\begin{table}%t3
%\centering
\par
\caption{\label{tab.kaaret} Coincidences between the WeCAPP catalogue
of variable stars and the X-ray selected catalogue of point sources by
\cite{kaaret02}. A search radius of 1$\arcsec$ was used. We give the
identifier and WCS coordinates for the WeCAPP sources, and the
identifier for the \cite{kaaret02} sources. For sources coincident
with the 2MASS catalogue \cite{cutri00}, we give the 2MASS identifier
also. We also show the difference $\Delta$$r$ of the matching of both catalogues
for each of the correlated sources. 
}
\begin{tabular}{rrrccc}
\hline\hline
WeCAPP &  $\alpha$(2000) & $\delta$(2000) & Kaaret & 2MASS & $\Delta$$r$ (arcsec) \\
\hline
 10~578  &  0h42m10.30s  &   41d15$\arcmin$10.4$\arcsec$  &   J004210.2+411510       & 0042102+411510   &  0.5      \\
 16~262  &  0h42m12.14s  &   41d17$\arcmin$58.8$\arcsec$  &   J004212.1+411758       & 0042121+411758   &  0.4      \\
  8624  &  0h42m18.68s  &   41d14$\arcmin$01.8$\arcsec$  &   J004218.6+411402       & 0042186+411402   &  0.5      \\
  8946  &  0h42m21.58s  &   41d14$\arcmin$19.8$\arcsec$  &   J004221.5+411419       & 0042215+411419   &  0.4      \\
  7582  &  0h42m25.11s  &   41d13$\arcmin$40.7$\arcsec$  &   J004225.1+411340       &                  &  0.6      \\
 19~068  &  0h42m31.26s  &   41d19$\arcmin$38.7$\arcsec$  &   J004231.2+411938       & 0042312+411938   &  0.2      \\
  7979  &  0h42m36.59s  &   41d13$\arcmin$49.9$\arcsec$  &   J004236.6+411350       &           &  0.7      \\
  9082  &  0h42m39.60s  &   41d14$\arcmin$28.6$\arcsec$  &   J004239.5+411428       &           &  0.9      \\
 11~406  &  0h42m41.45s  &   41d15$\arcmin$23.9$\arcsec$  &   J004241.4+411524       &           &  0.3      \\
 16~322  &  0h42m43.97s  &   41d17$\arcmin$55.5$\arcsec$  &   J004243.9+411755       &           &  0.4      \\
 15~344  &  0h42m44.88s  &   41d17$\arcmin$39.5$\arcsec$  &   J004244.8+411740       &           &  0.4      \\
 12~503  &  0h42m46.99s  &   41d16$\arcmin$15.3$\arcsec$  &   J004246.9+411615       &           &  0.7      \\
  8501  &  0h42m47.13s  &   41d14$\arcmin$13.9$\arcsec$  &   J004247.1+411413       &           &  0.8      \\
 10~431  &  0h42m47.45s  &   41d15$\arcmin$07.6$\arcsec$  &   J004247.4+411507       &           &  0.2      \\
 11~736  &  0h42m47.90s  &   41d15$\arcmin$50.6$\arcsec$  &   J004247.8+411550       &           &  0.6      \\
 12~891  &  0h42m48.65s  &   41d16$\arcmin$25.0$\arcsec$  &   J004248.6+411624       &           &  0.7     \\
 20~170  &  0h42m55.27s  &   41d20$\arcmin$45.1$\arcsec$  &   J004255.3+412045       &           &  0.7     \\
 18~374  &  0h42m59.66s  &   41d19$\arcmin$19.3$\arcsec$  &   J004259.6+411919       &           &  0.3      \\
 12~404  &  0h42m59.88s  &   41d16$\arcmin$06.0$\arcsec$  &   J004259.8+411606       &           &  0.1      \\
 21~059  &  0h43m03.31s  &   41d21$\arcmin$21.8$\arcsec$  &   J004303.2+412121       &           &  0.5      \\
  6049  &  0h43m08.42s  &   41d12$\arcmin$46.9$\arcsec$  &   J004308.4+411247       &           &  0.7      \\
 17~815  &  0h43m09.88s  &   41d19$\arcmin$00.8$\arcsec$  &   J004309.8+411900       &           &  0.7     \\
  9991  &  0h43m10.62s  &   41d14$\arcmin$51.3$\arcsec$  &   J004310.5+411451       & 0043106+411451 &   0.5     \\
\hline
\end{tabular}
\end{table}