\begin{table}%T2
\caption{\label{tabel1}Stellar variability classes and the code abbreviation used in
Paper~I.}
 \small%\centering
\par
\begin{tabular}{cc}
  \hline\hline
    Class& Abbreviation \\
  \hline
  Periodically variable supergiants  & PVSG \\
  Pulsating Be-stars & BE\\
  $\beta$-Cephei stars & BCEP \\
  Classical Cepheids & CLCEP \\
  Beat (double-mode)-Cepheids & DMCEP \\
  Population II Cepheids & PTCEP \\
  Chemically peculiar stars & CP \\
  $\delta$-Scuti stars & DSCUT \\
  $\lambda$-Bootis stars & LBOO \\
  SX-Phe stars & SXPHE \\
  $\gamma$-Doradus stars & GDOR \\
  Luminous Blue Variables & LBV \\
  Mira stars & MIRA \\
  Semi-Regular stars & SR \\
  RR-Lyrae, type RRab & RRAB \\
  RR-Lyrae, type RRc & RRC \\
  RR-Lyrae, type RRd & RRD \\
  RV-Tauri stars & RVTAU \\
  Slowly-pulsating B stars & SPB \\
  Solar-like oscillations in red giants & SLR \\
  Pulsating subdwarf B stars & SDBV \\
  Pulsating DA white dwarfs & DAV \\
  Pulsating DB white dwarfs & DBV \\
  GW-Virginis stars & GWVIR \\
  Rapidly oscillating Ap stars & ROAP \\
  T-Tauri stars & TTAU \\
  Herbig-Ae/Be stars & HAEBE \\
  FU-Ori stars & FUORI \\
  Wolf-Rayet stars & WR \\
  X-Ray binaries & XB \\
  Cataclysmic variables & CV \\
  Eclipsing binary, type EA & EA \\
  Eclipsing binary, type EB & EB \\
  Eclipsing binary, type EW & EW \\
  Ellipsoidal binaries & ELL \\
  \hline
\end{tabular}
\end{table}