\begin{table}%t3
\caption{\label{table-Prot}Photometric periods and ancillary data are presented, resulting from the light-curve analysis of variable stars detected in the Lowell M~34 fields.}
\par
%\centering
 {
\begin{tabular}{lrrrrl}
\hline\hline \noalign{\smallskip}
Internal\tablefootmark{a}  ~~    & Data\tablefootmark{b} & Sigma Clipped\tablefootmark{c} & Period 
                    & $B-V_{o}$\tablefootmark{d} & Mem\tablefootmark{e} \\
Identifier  & Epochs & StdDev [mag] & [days] & &  \\
\hline
  F3\_0172-lIlVsV   & 53/54/59     & 0.00883/0.01010/0.01190          & $ 8.0    \pm  1.0  $ & 0.811 & Y;Ys \\
  F3\_0176-lIlVsIsV & 53/54/58/59  & 0.04275/0.06460/0.04313/0.06427  & $ 2.780  \pm  0.005$ & 0.818 & Y;Ys \\
  F3\_0215-lIlVsIsV & 52/54/58/59  & 0.01121/0.01722/0.01439/0.02020  & $ 7.47   \pm  0.11 $ & 0.874 & Y;Ys \\
  F3\_0258-lIlVsV   & 53/54/58     & 0.01182/0.01250/0.01457          & $11.0    \pm  1.0  $ & 0.947 & Y;Ys \\
  F3\_0306-lIsIsV   & 53/58/59     & 0.01886/0.01809/0.02081          & $1.1435  \pm 0.0007$ & 0.991 & Y;Yb \\
  F3\_0320-lIlVsV   & 52/54/58     & 0.00898/0.01023/0.01430          & $ 8.511  \pm 0.001 $ & 1.046 & Y;   \\
  F3\_0383-lIlV     & 52/54        & 0.00776/0.00937                  & $ 9.5    \pm  0.4  $ & 1.160 & Y;Ys \\
  F3\_0430-lV       & 54           & 0.01253                          & $10.5    \pm 1.0   $ & 1.239 & Y;Ys \\
  F3\_0469-lIlVsIsV & 52/54/57/57  & 0.01344/0.01745/0.01768/0.02225  & $12.9    \pm  0.3  $ & 1.283 & Y; \\
  F3\_0485-lIlV     & 52/54        & 0.01040/0.01393                  & $12.0    \pm  1.0  $ & 1.285 & Y; \\
  F3\_0487-lIlV     & 53/54        & 0.01076/0.01388                  & $ 8.4    \pm  0.6  $ & 1.278 & Y; \\
  F3\_0600-lIlV     & 53/54        & 0.01263/0.02503                  & $ 7.44   \pm  0.05 $ & 1.452 & Y; \\
  F3\_0664-lI       & 52           & 0.01077                          & $10.5    \pm 1.0   $ & 1.441 & Y; \\
  F4\_0136-sIsV     & 60/60        & 0.01457/0.01794                  & $ 2.87   \pm  0.03 $ & 0.544 & Y;Ys \\ 
  F4\_0169-lIlVsIsV & 55/42/60/59  & 0.01275/0.01297/0.01094/0.01429  & $ 3.81   \pm  0.08 $ & 0.598 & Y;Ys \\ 
  F4\_0194-sIsV     & 60/60        & 0.00817/0.00889                  & $ 2.20   \pm  0.03 $ & 0.652 & Y;Ys \\ 
  F4\_0234-lIlVsV   & 54/55/60     & 0.00692/0.00984/0.01014          & $ 5.56   \pm  0.07 $ & 0.698 & Y;Ys \\ 
  F4\_0303-lIlVsIsV & 55/55/60/60  & 0.00800/0.00941/0.00839/0.00978  & $ 7.4    \pm  0.3  $ & 0.767 & Y;Ys \\ 
  F4\_0317-lIlVsIsV & 55/55/59/60  & 0.01701/0.02159/0.01698/0.02167  & $ 6.8    \pm  0.1  $ & 0.805 & Y;Ys \\ 
  F4\_0327-lVsV     & 55/60        & 0.01471/0.01406                  & $ 7.6    \pm  1.1  $ & 0.813 & Y;Ys \\ 
  F4\_0335-lIlVsIsV & 55/55/60/60  & 0.01538/0.01953/0.01601/0.02032  & $ 0.89   \pm  0.02 $ & 0.790 & Y;Yb \\ 
  F4\_0450-lIlVsIsV & 54/55/60/60  & 0.00985/0.01181/0.01264/0.01368  & $ 8.00   \pm  0.21 $ & 0.895 & Y;Ys \\ 
  F4\_0667-lIlVsV   & 54/55/59     & 0.01122/0.01819/0.02028          & $ 7.97   \pm  0.05 $ & 1.030 & Y;Yb \\ 
  F4\_0695-lI       & 54           & 0.00748                          & $ 4.3    \pm 0.5   $ & 1.086 & Y;Ys \\
  F4\_0730-lIlVsIsV & 55/55/60/59  & 0.02944/0.04619/0.03109/0.04695  & $ 8.41   \pm  0.10 $ & 1.051 & Y; \\
  F4\_0736-lIlVsIsV & 55/55/60/60  & 0.01875/0.02715/0.02022/0.02911  & $ 0.786  \pm  0.001$ & 1.008 & Y;Yb \\ 
  F4\_0803-lVsI     & 55/60        & 0.01435/0.01416                  & $12.6    \pm  0.7  $ & 1.164 & Y;Ys \\ 
  F4\_0804-lIlVsIsV & 55/55/60/60  & 0.02568/0.04152/0.02448/0.04239  & $ 4.95   \pm  0.04 $ & 1.106 & Y; \\
  F4\_0852-lIlVsIsV & 55/55/59/60  & 0.01547/0.02368/0.01624/0.02564  & $0.879   \pm  0.002$ & 1.155 & Y;Yb \\ 
  F4\_0942-lIlVsV   & 54/55/60     & 0.00942/0.01300/0.02362          & $ 9.4    \pm  0.3  $ & 1.198 & Y; \\
  F4\_1007-lIlV     & 55/55        & 0.00774/0.01177                  & $15      \pm 2     $ & 1.440 & Y; \\ 
  F4\_1020-lIlVsIsV & 55/55/60/59  & 0.01344/0.01846/0.01568/0.02528  & $ 8.6    \pm  0.4  $ & 1.260 & Y; \\
  F4\_1055-lIlVsIsV & 55/55/60/60  & 0.01427/0.02542/0.02233/0.02664  & $ 6.80   \pm  0.15 $ & 1.272 & Y; \\
  F4\_1147-lV       & 55           & 0.01883                          & $ 0.589  \pm 0.001 $ & 1.336 & Y; \\
  F4\_1315-lIlV     & 54/54        & 0.01429/0.01913                  & $12.2    \pm  0.5  $ & 1.371 & Y; \\
  F4\_1357-lIlV     & 55/55        & 0.01197/0.01973                  & $ 9.4    \pm  0.2  $ & 1.380 & Y; \\
  F4\_1369-lIlV     & 53/53        & 0.01886/0.02578                  & $11.85   \pm  0.13 $ & 1.443 & Y; \\
  F4\_1392-lIlV     & 55/55        & 0.01496/0.02385                  & $ 6.5    \pm  0.5  $ & 1.434 & Y; \\
  F4\_1566-lIlV     & 55/54        & 0.01920/0.03248                  & $11.2    \pm  0.1  $ & 1.479 & Y; \\
  F4\_1617-lV       & 52           & 0.03379                          & $ 7.3    \pm 0.5   $ & 1.500 & Y;  \\
  F4\_1793-lIlV     & 55/53        & 0.02221/0.04966                  & $ 7.5    \pm  0.6  $ & 1.323 & Y; \\
  F4\_1925-lV$^{f}$ & 44           & 0.09210                          & $12.7    \pm 2.0   $ & 1.507 & Y;  \\
  F4\_2226-lI$^{f}$ & 55           & 0.02681                          & $ 6.0    \pm 0.5   $ & 1.555 & Y;  \\ \hline
  F3\_0071-sIsV     & 58/59        & 0.02052/0.02502                  & $ 3.014  \pm 0.008 $ & 0.977 & N;  \\
  F3\_0121-lVsV     & 54/59        & 0.00851/0.00881                  & $ 8.4    \pm 0.2   $ & 1.178 & N; \\
  F3\_0163-lIsIsV   & 53/58/59     & 0.00814/0.00943/0.00935          & $14      \pm  2    $ & 0.830 & Y;N \\
  F3\_0165-lI       & 52           & 0.01089                          & $12      \pm 1     $ & 0.795 & Y;N \\
  F3\_0388-lIlVsIsV & 53/54/58/59  & 0.01534/0.02141/0.01715/0.02448  & $11.59   \pm 0.01  $ & 0.905 & N; \\
  F3\_0413-lIlVsIsV & 53/54/58/59  & 0.01640/0.02417/0.01909/0.02982  & $ 5.45   \pm  0.08 $ & 1.073 & Y;N \\
  F3\_0437-lIlVsV   & 53/54/59     & 0.00859/0.01134/0.01563          & $ 9.7    \pm 0.4   $ & 0.577 & N; \\
  F3\_0692-lIlV     & 53/54        & 0.01886/0.02686                  & $ 0.3368 \pm 0.0001$ & 0.787 & N; \\
  F3\_2310-lIlV     & 52/54        & 0.02667/0.02846                  & $ 2.991  \pm 0.008 $ & - - - & \\
  F4\_0167-lIlVsI   & 54/55/59     & 0.01321/0.01091/0.00961          & $ 9.2    \pm 0.9   $ & 0.868 & N; \\
  F4\_0404-lIlVsV   & 55/55/60     & 0.01099/0.01419/0.01461          & $ 6.6    \pm  0.3  $ & 0.782 & Y;N \\
  F4\_0515-lIlVsV   & 55/55/60     & 0.00886/0.00957/0.01239          & $ 8.2    \pm 0.1   $ & 0.833 & N; \\
\hline
\end{tabular}}
\tablefoot {\tablefoottext{a}{Internal Identifiers are the same as those detailed in Table~\ref{table-identifier}. Designations indicating exposure time and filter choice for a given light-curve are annotated. For instance, {lI} represents {\em long-I}, for light-curves derived from long exposures in the $I$-filter. Thus, {lIlVsIsV} represents four independent light-curves created from image sequences of 400~s, $I$-filter; 600~s, $V$-filter; 40~s, $I$-filter and 60~s, $V$-filter, respectively (namely, long-I, long-V, short-I \& short-V).}\\
\tablefoottext{b}{Number of photometric data points in each light-curve, derived from each target's image series, in a given filter and exposure time sequence.} \\
\tablefoottext{c}{For each target's light-curve, in a filter+exposure combination, standard deviations of the differential magnitudes are provided. The time series files for each target were sigma-clipped to eliminate outliers. A $\Delta$-magnitude for each light-curve can be determined by multiplying these standard deviations by~2$\sqrt2$ (strictly speaking this is only true for perfectly sinusoidal variations).} \\
\tablefoottext{d}{$E_{B-V}$~= 0.07 is adopted; Canterna et~al. (\cite{Cant79}).} \\
\tablefoottext{e}{Abridged cluster membership criteria are reproduced from Table~\ref{table-identifier}, with format Photometric; Kinematic (s-single, b-binary).} \\
\tablefoottext{f}{$B-V$ colours are determined using a field  star $V-I$ to $B-V$ relationship (Caldwell et~al. \cite{Cald93}), assuming $E_{V-I}$~$=$ $1.25$~$\times$ $E_{B-V}$, and $E_{B-V}$~=~0.07.}}
\end{table}