\begin{table}%t4
%\centering
\par
%\begin{footnotesize}
\caption{The variables in the {\em NOT01} field. The first column contains the variable name, 
where the new variables
are printed with {\em italics} ({\em V79--V100}). Columns 2--4 contain ID, right ascension, and 
declination from Stetson \ea~(\cite{stetson03}). Columns 5 and 6 are the periods and amplitudes (in the $V$ filter) 
we have determined.
The last column gives the variable star type. The positions of the variables in the colour-magnitude
diagram are given in Figs.~\ref{fig:cmd_n6791_transits} and~\ref{fig:cmd_n6791_vars} while the
phased light curves of some of the stars are shown in Figs.~\ref{fig:n6791_known}, \ref{fig:n6791_new},
and~\ref{fig:V09}.
\label{tab:n6791_var}}
%\vskip 0.2cm
\begin{tabular}{rr|cc|rrl} %%%%%%%%%%%%%%%% FOR ID vs ID check this FILE: /M4/n6791/n6791_fundamental3.dat %%%%%%%%%%%%%%%%%%%%%%%5
\hline\hline
Name & ID & $\alpha_{2000.0}$ & $\delta_{2000.0}$ & \multicolumn{1}{c}{$P$ [days]} & \multicolumn{1}{c}{$A$ [mag]}   & \multicolumn{1}{c}{Var.\ type} \\
\hline
   V1    &  6271   & 19$^{\rm h}$20$^{\rm m}$47\fs61&$ +$37$^\circ$44\Secc32\farcs0  & 0.2676766 &    0.194 &  EB, close \\  % 0.2676765 &    0.152 &  0.763
   V4    &  8576   & 19$^{\rm h}$20$^{\rm m}$54\fs22&$ +$37$^\circ$48\Secc23\farcs8  & 0.325667  &    0.046 &  EB, close \\  % 0.325642  &    0.038 &  0.204 
   V5    &  5883   & 19$^{\rm h}$20$^{\rm m}$46\fs53&$ +$37$^\circ$48\Secc47\farcs9  & 0.312666  &    0.017 &  EB, close \\  % 0.312703  &    0.017 &  0.441
   V6    & 11376   & 19$^{\rm h}$21$^{\rm m}$02\fs72&$ +$37$^\circ$48\Secc49\farcs1  & 0.279062  &    0.042 &  EB, close \\
   V9    &  6371   & 19$^{\rm h}$20$^{\rm m}$47\fs88&$ +$37$^\circ$46\Secc37\farcs4  & 3.19174   &    0.040$^{a}$ &  EB, close \\  
  V16    & 12695   & 19$^{\rm h}$21$^{\rm m}$07\fs59&$ +$37$^\circ$48\Secc09\farcs6  & 4.53      &    0.026 &  EB, close \\  
  V31    & 11307   & 19$^{\rm h}$21$^{\rm m}$02\fs47&$ +$37$^\circ$47\Secc09\farcs3  & 3.34154   &    0.015 &  EB, close \\
  V33    &  3886   & 19$^{\rm h}$20$^{\rm m}$39\fs81&$ +$37$^\circ$43\Secc54\farcs4  & 2.35944   &    0.040 &  EB, close \\  
  V38    & 11652   & 19$^{\rm h}$21$^{\rm m}$03\fs69&$ +$37$^\circ$46\Secc05\farcs9  & 3.845     &    0.023 &  EB, close \\  \hline
  V20    &  8600   & 19$^{\rm h}$20$^{\rm m}$54\fs30&$ +$37$^\circ$45\Secc34\farcs7  &14.4698    &    0.3$^{a}$ &  EB, detached \\ % NOT01 ID = 335
  V60    & 10746   & 19$^{\rm h}$21$^{\rm m}$00\fs70&$ +$37$^\circ$45\Secc45\farcs1  & 7.510/7.1$^{b}$ &    0.4/0.015$^{b}$ &  EB, detached \\ % NOT01 =1411
{\em V79}&  8943    & 19$^{\rm h}$20$^{\rm m}$55\fs21&$ +$37$^\circ$46\Secc39\farcs7  & $\sim$9.0038   &    0.15$^{a}$ &  EB, detached \\ % \hline % VAR14=1347 
{\em V80}$^{c}$
         & 12390   & 19$^{\rm h}$21$^{\rm m}$06\fs48&$ +$37$^\circ$47\Secc27\farcs8  & 4.447     & 0.014    &  EB? \\ \hline % %{\em V80 = T9}$^{c}$ % VAR8 = 789 (DAOID)
  V14    &  7637   & 19$^{\rm h}$20$^{\rm m}$51\fs67&$ +$37$^\circ$45\Secc24\farcs8  & 5.4--5.8  & 0.028    &  Periodic Var. \\ % VAR15
  V17    &  3626   & 19$^{\rm h}$20$^{\rm m}$38\fs88&$ +$37$^\circ$49\Secc04\farcs6  & 6.42566   & 0.036    &  Periodic Var. \\
  V41    &  7397   & 19$^{\rm h}$20$^{\rm m}$50\fs97&$ +$37$^\circ$48\Secc24\farcs8  & 0.4807278 & 0.039    &  Periodic Var. \\
  V53    & 10798   & 19$^{\rm h}$21$^{\rm m}$00\fs84&$ +$37$^\circ$44\Secc35\farcs4  & 7.815     & 0.039    &  Periodic Var. \\ % 7.61--8.02& 0.039    &          
{\em V81}&  3268   & 19$^{\rm h}$20$^{\rm m}$49\fs65&$ +$37$^\circ$48\Secc08\farcs7  & 7.58      & 0.008    &  Periodic Var. \\ % I14
{\em V82}&  3857   & 19$^{\rm h}$20$^{\rm m}$39\fs71&$ +$37$^\circ$47\Secc36\farcs1  & 7.58886   & 0.010    &  Periodic Var. \\ % FGJ18 6.55596   & 0.021    & 
{\em V83}&  5848   & 19$^{\rm h}$20$^{\rm m}$46\fs40&$ +$37$^\circ$44\Secc14\farcs1  & 7.014     & 0.037    &  Periodic Var. \\ % VAR20 6.991     & 0.048 
{\em V84}&  6305   & 19$^{\rm h}$20$^{\rm m}$47\fs71&$ +$37$^\circ$44\Secc58\farcs2  & 1.6333    & 0.03     &  Periodic Var. \\ % VAR21
{\em V85}&  7011   & 19$^{\rm h}$20$^{\rm m}$49\fs86&$ +$37$^\circ$45\Secc50\farcs9  & 4.100     & 0.007    &  Periodic Var., EB? \\ % FGJ22
{\em V86}&  7099   & 19$^{\rm h}$20$^{\rm m}$50\fs13&$ +$37$^\circ$48\Secc31\farcs7  & 7.39      & 0.011    &  Periodic Var. \\ % BR53
{\em V87}&  8033   & 19$^{\rm h}$20$^{\rm m}$52\fs78&$ +$37$^\circ$44\Secc58\farcs8  & 6.971     & 0.006    &  Periodic Var. \\  % VAR12
{\em V88}&  8088   & 19$^{\rm h}$20$^{\rm m}$52\fs91&$ +$37$^\circ$46\Secc36\farcs9  & 6.91      & 0.008    &  Periodic Var. \\ % I11
{\em V89}&  9432   & 19$^{\rm h}$20$^{\rm m}$56\fs64&$ +$37$^\circ$46\Secc36\farcs2  & 5.7617    & 0.028    &  Periodic Var. \\ % VAR16 
{\em V90}& 10169   & 19$^{\rm h}$20$^{\rm m}$58\fs86&$ +$37$^\circ$44\Secc47\farcs2  & 5.71      & 0.008    &  Periodic Var. \\ % I34
{\em V91}& 10699   & 19$^{\rm h}$21$^{\rm m}$00\fs54&$ +$37$^\circ$48\Secc40\farcs7  & 5.13      & 0.011    &  Periodic Var. \\ % I32
{\em V92}& 11380   & 19$^{\rm h}$21$^{\rm m}$02\fs73&$ +$37$^\circ$46\Secc00\farcs8  & 7.24      & 0.008    &  Periodic Var. \\ % I35
{\em V93}& 12049   & 19$^{\rm h}$21$^{\rm m}$05\fs23&$ +$37$^\circ$47\Secc08\farcs5  & 0.94928   & 0.007    &  Periodic Var. \\ \hline % VAR11  0.94928   & 0.02 
  B7     & 12652   & 19$^{\rm h}$21$^{\rm m}$07\fs40&$ +$37$^\circ$47\Secc56\farcs5  &$\sim$13.3 & 0.15     &  Long period \\  %$\sim$13   & 0.4      & 
  V62    & 11475   & 19$^{\rm h}$21$^{\rm m}$03\fs06&$ +$37$^\circ$43\Secc51\farcs8  &$\sim$17   & 0.027    &  Long period \\
  V65    &  7920   & 19$^{\rm h}$20$^{\rm m}$52\fs47&$ +$37$^\circ$47\Secc30\farcs5  & 8.613     & 0.008    &  Long period \\ % 8.891     & 0.01
  V67    & 11645   & 19$^{\rm h}$21$^{\rm m}$03\fs67&$ +$37$^\circ$48\Secc03\farcs7  &$\sim$10   & 0.05     &  Long period \\
  V73    &  8108   & 19$^{\rm h}$20$^{\rm m}$52\fs97&$ +$37$^\circ$46\Secc52\farcs5  &$\sim$20.9 & 0.02     &  Long Period \\ % I0 = once was V87
{\em V94}&  4640   & 19$^{\rm h}$20$^{\rm m}$42\fs50&$ +$37$^\circ$44\Secc36\farcs9  &$\sim$15.57& 0.01     &  Long period \\ % VAR5
{\em V95}&  4805   & 19$^{\rm h}$20$^{\rm m}$43\fs05&$ +$37$^\circ$47\Secc32\farcs5  & 9.477     & 0.012    &  Long period \\ % VAR17
{\em V96}&  5485   & 19$^{\rm h}$20$^{\rm m}$45\fs26&$ +$37$^\circ$45\Secc48\farcs8  & 9.307     & 0.012    &  Long Period \\ %  FGJ3
{\em V97}&  6777   & 19$^{\rm h}$20$^{\rm m}$49\fs17&$ +$37$^\circ$49\Secc14\farcs8  & 9.563     & 0.013    &  Long period \\ % VAR1
{\em V98}&  9353   & 19$^{\rm h}$20$^{\rm m}$56\fs42&$ +$37$^\circ$45\Secc38\farcs4  &$\sim$8.99 & 0.01     &  Long period \\ %  VAR7
{\em V99}&  9568   & 19$^{\rm h}$20$^{\rm m}$57\fs06&$ +$37$^\circ$48\Secc12\farcs2  &$\sim$10   & 0.003    &  Long period \\ % VAR4
{\em V100}&11111   & 19$^{\rm h}$21$^{\rm m}$01\fs81&$ +$37$^\circ$45\Secc42\farcs0  &12.5215    & 0.01     &  Long period \\ % VAR3  &12.5215    & 0.037 
\hline
\multicolumn{7}{l}{$^a$ For the eclipsing binaries V9, V20, and {\em V79} 
the depth of the primary eclipse in the $V$ filter is given.} \\
\multicolumn{7}{l}{$^b$ V60 is variable with a low amplitude
and a period of $P\sim7.1$~days while the period estimated from the} \\
\multicolumn{7}{l}{secondary and primary eclipses is $7.510\pm0.005$~days. The primary eclipse depth is 0.4~mag in $V$.} \\
\multicolumn{7}{l}{$^c$ {\em V80} was detected in our search for transit-like events and is also 
given the name {\em T9} (cf  Fig.~\ref{fig:planet_transits}).}\\
\multicolumn{7}{l}{Furthermore, {\em V80} is variable with a low amplitude.} \\
%\multicolumn{7}{l}{} \\
\end{tabular}
%\end{footnotesize}
\end{table}