\begin{table}%t1
\caption{The LPVs of 47~Tuc.\label{variables}} 
%\centerline
{\begin{tabular}{lccccccccc}
\hline \hline 
Name & $\alpha$ (2000) & $\delta$ (2000) & $V$ & $V-I_{\rm c}$ & $J$ & $K$ & $P$ [d] & $P_{\rm literature}$ & Remark\\
\hline 
\noalign{\smallskip}
V1   & 00 24 12.4  & $-$72 06 39 & 13.15 &  3.86 & 7.45 & 6.21 & 221 & 212 & 1\\
V2   & 00 24 18.4  & $-$72 07 59 &   --    &   --   & 7.52 & 6.29 & 203 & 203 & 1, 2\\
V3   & 00 25 15.9  & $-$72 03 54 & 12.63  &  3.54  & 7.49 & 6.27 & 192 & 192 & 1   \\
V4   & 00 24 00.3  & $-$72 07 26 & 12.34 &  2.62 & 7.87 & 6.69 & 165 & 82, 165 & 1, 3 \\
V5   & 00 25 03.7  & $-$72 09 31 & 11.80  &  1.99  & 8.65 & 7.47 & 50 & 60 & 1, 4  \\
V6   & 00 24 25.5  & $-$72 06 30 & 11.74 &  1.94 & 8.54 & 7.43 & 48 & 48 & 1  \\
V7   & 00 25 20.6  & $-$72 06 40 & 11.83  &  2.30  & 8.18 & 6.97 & 52 & 52 & 1, 4    \\
V8   & 00 24 08.3  & $-$72 03 54 & 12.01 &  2.39 & 7.94 & 6.70 & 155 & 155 & 1    \\
V11  & 00 25 09.0  & $-$72 02 17 & 12.03  &  2.70  & 7.91 & 6.71 & 160: & 52, 100 & 4, 5\\
V13  & 00 22 58.3  & $-$72 06 56 & 12.36  &  2.23  & 8.79 & 7.70 & 40 + long & 40 & 1, 4, 8\\
V16  & 00 25 23.2  & $-$72 11 05 & 11.65  &  2.0   & 8.35 & 7.23 & 41, 88: & 45 & \\
V18  & 00 25 09.2  & $-$72 02 39 & 11.67  &  1.95  & 8.59 & 7.47 & 83:  & & 1, 4\\
V19  & 00 24 14.8  & $-$72 04 44 & 11.46 &  1.70 & 8.79 & 7.61 & 83 & & \\
V20  & 00 24 14.5  & $-$72 05 09 & 12.30   &  2.53 & 8.08 & 6.94 & 232: & & 11\\
V21  & 00 23 50.1  & $-$72 05 50 & 12.41 &  2.85 & 8.07 & 6.78 & 76: + long & & 1   \\
V22  & 00 24 08.9  & $-$72 03 00 & 11.80 &  1.99 & 8.38 & 7.18 & 62 & & 8 \\
V23  & 00 24 29.5  & $-$72 09 08 & 11.77 &  2.08 & 8.68 & 7.53 & 52 + long & & \\
V25  & 00 23 58.9  & $-$72 02 35 & 11.96 &  2.50 & 8.20 & 7.03 & 44 & 42 & 9\\
V27  & 00 24 15.2  & $-$72 04 36 & 12.11  &  2.52  & 7.97 & 6.77 & 69 + long & & \\
A19  & 00 24 21.8  & $-$72 04 13 & 12.18 &  2.57 & 8.08 & 6.79 & 60 & & \\
LW1  & 00 23 22.3  & $-$72 05 40 & 11.83 &  2.08 & 8.39 & 7.19 & 39 & & 9\\ %lc149%
LW2  & 00 23 29.2  & $-$72 06 20 & 11.90 &  2.23 & 8.26 & 7.05 & 60 + long & & 9\\ %F3lc137%
LW3  & 00 23 47.4  & $-$72 06 53 & 11.92 &  2.35 & 8.13 & 6.89 & 107 & & \\%F4lc243%
LW4  & 00 23 51.3  & $-$72 03 49 & 11.80   &  1.98 & 8.56 & 7.37 & 32 + long: & & 9\\%F4lc238
LW5  & 00 23 53.2  & $-$72 04 16 & 11.74 &  1.96 & 8.53 & 7.32 & 40 & & \\ %lc80%
LW6  & 00 23 54.7  & $-$72 03 39 & 11.85  &  2.00 & 8.51 & 7.30 & 41 & & 9\\ %F4lc231
LW7  & 00 23 56.9  & $-$72 05 33 & 11.66 &  1.86 & 8.26 & 7.18 & 42 & & 10\\ %lc73 - O4%
LW8  & 00 23 57.7  & $-$72 05 30 & 11.82 &  1.88 & 8.10 & 7.12 & 27: + long & & 9\\ %lc72%
LW9  & 00 23 58.2  & $-$72 05 49 & 12.34 &  2.77 & 7.97 & 6.74 & 74 & & 9\\ %lc69%
LW10 & 00 24 02.6  & $-$72 05 07 & 12.22 &    --   & 7.57 & 6.40 & 110:, 221: & & 2, 10, 11\\ %O1%
LW11 & 00 24 03.2  & $-$72 04 51 & 11.95 &  1.79 & 8.47 & 7.40 & 36: & & 11\\ %F3lc59%
LW12 & 00 24 04.0  & $-$72 05 10 & 11.96 &  2.35 & 8.12 & 6.89 & 61, 116 & & 11\\ %lc56
LW13 & 00 24 07.9: & $-$72 04 32:& 12.56 &  2.93 & 7.44: & 6.25: & 65: & & 6, 11\\ %F3lc54%
LW14 & 00 24 09.4: & $-$72 04 49:& 11.71 &  1.99 & 8.42 & 7.39 & 50 & & 7, 10\\ %O3%
LW15 & 00 24 11.2  & $-$72 05 09 & 11.76 &  2.05 & 8.32 & 7.13 & 46 + long & & 9\\ %lc45%
LW16 & 00 24 13.6  & $-$72 04 52 & 11.88 &  1.89 & 8.39 & 7.32 & 29 + long & & 9 \\ %lc41%
LW17 & 00 24 16.3  & $-$72 01 31 & 11.81  &  1.99 & 8.43 & 7.20 & 41 & & 9\\ %F4lc161
LW18 & 00 24 20.5  & $-$72 04 50 & 11.91  &  2.33 & 7.95 & 6.77 & 65 + long & & \\ %F4lc139%
LW19 & 00 24 23.2  & $-$72 04 23 & 11.85 &  2.17 & 8.38 & 7.16 & 40 + long & & 9, 10 \\ %O5%
LW20 & 00 24 52.1  & $-$71 56 11 &   --    &   --   & 8.31 & 7.11 & 49 & & 2, 8\\ %MACHO1222%
LW21 & 00 25 23.2  & $-$72 11 05 &   --    &   --    & 8.44 & 7.28 & 38 & & 2, 8\\ %MACHO786%
LW22 & 00 25 30.1  & $-$72 04 32 & 12.06 &  2.48 & 8.16 & 6.93 & 63 + long & & \\
\hline
\end{tabular}}
\par
\smallskip
Notes: Cols.~2 and~3 give coordinates from 2MASS. Column~4 is the mean $V$ brightness.
$J$ and $K$ colours are from 2MASS converted to the AAO system, if not stated otherwise. 
If there is an indication for
a long secondary period exceeding the time span of the monitoring, the star is
marked with "+long''. Uncertain values are marked with a colon.\\
Remarks: (1) see Lebzelter et~al. (\cite{LWHJF05}); (2) no $V$ or $V-I_{\rm c}$, not in the CMD (Fig.~\ref{lctime}); 
(3) currently only the longer period is
visible; (4) photometry in the CMD from Fox (\cite{fox82}) -- see text; (5) current periodicity
unclear, see Lebzelter et~al. (\cite{LWHJF05}) for details; (6) close neighbour on 2MASS images, 
NIR fluxes and position possibly wrong; (7) not in 2MASS point source catalogue, 
coordinates calculated from our images, $K$ magnitude from
Origlia et~al. (\cite{origlia02}); (8) only on Mount Stromlo frames; (9) no Mount Stromlo data; 
(10) stars with near infrared excess detected by Origlia et~al. (\cite{origlia02}); 
(11) see text in Sect.~\ref{var_section} for comments on the periods.
\end{table}