\begin{table}%T5 \caption{\label{tbl:limits}Truncated version of the catalogue of sdB stars observed during our search programme.} \small%\centering \par \begin{tabular}{llccccrrrrl} \hline\hline\noalign{\smallskip} Target Name & Other Name & RA & Dec & \mpg & Run &$N_{\rm p}$&$\Delta t$&$\sigma$& $A_{\rm max}$ & Var \\ & & J2000 & J2000 & mag & & & s & mma & mma & \\ \hline SB~7 & MCT~0000--1637 & 00:03:24.37 & $-$16:21:06.3 & 12.7 & S5 & 60 & 20 & 0.60 & 1.26 & NOV \\ HE~0002--2648 & MCT~0002--2648 & 00:05:09.58 & $-$26:31:48.4 & 15.6 & S5 & 39 & 20 & 1.01 & 2.07 & NOV \\ HE~0004--2737 & MCT~0004--2737 & 00:06:46.26 & $-$27:20:53.4 & 13.7 & N4 & 60 & 20 & 0.44 & 0.95 & NOV \\ HE~0007--2212 & MCT~0007--2737 & 00:09:45.91 & $-$21:56:14.4 & 14.9 & S5 & 43 & 10 & 0.79 & 1.48 & NOV \\ MCT~0008--1245 & ... & 00:11:25.04 & $-$12:28:45.9 & 14.3 & S4 & 93 & 15 & 0.59 & 1.04 & NOV \\ \noalign{\smallskip} KUV~04233+1502 & ... & 04:26:08.00 & +15:08:29.01 & 14.3 & S4 & 129 & 20 & 0.33 & 1.01 & \\ KPD~0716+0258 & ... & 07:18:57.85 & +02:53:14.67 & 14.7 & T4 & 270 & 30 & 0.25 & 0.78 & \\ KUV~07301+3659 & ... & 07:33:25.62 & +36:52:57.83 & 14.8 & S4 & 134 & 18 & 0.30 & 0.93 & \\ PG~1248+164 & ... & 12:50:50.23 & +16:10:03.40 & 14.0 & T7 & 65 & 20 & 5.07 &16.61 & \\ PG~1313+132 & ... & 13:15:58.16 & +12:57:40.42 & 14.1 & S6 & 96 & 20 & 0.95 & 3.35 & \\ J1351+0234 & ... & 13:51:40.69 & +02:34:29.21 & 17.1 & N7 & 70 & 30 & 0.91 & 2.93 & \\ PG~1722+286 & ... & 17:24:11.97 & +28:35:26.90 & 12.8 & N1 &1191 & 5 & 1.01 & 3.08 & \\ PG~1725+252 & ... & 17:27:57.39 & +25:08:35.70 & 12.7 & T2 & 61 & 10 & 3.38 &12.39 & \\ HS~2029+0301 & ... & 20:31:52.63 & +03:11:17.39 & 15.6 & N1 & 952 & 5 & 2.13 & 6.41 & \\ KPD~2215+5037 & ... & 22:17:20.62 & +50:52:58.09 & 13.6 & N5 & 45 & 25 & 0.69 & 2.39 & \\ \hline \end{tabular}\tablefoot{The full table with 285 entries is available in electronic form from at the CDS. Only the first five entries in the table are listed, plus the ten stars that have peaks between 3$\sigma$ and the 3.7$\sigma$ cutoff required for the NOV flag (discussed in Sect.~\ref{sect:pcand}). The stars in the sample for which pulsations were detected are listed in Table~\ref{tbl:sdbvars}. The columns include target names, coordinates, a magnitude estimate (usually photographic), the run ID from Table~\ref{tbl:obstime}, the number of data points in the light-curve ($N_{\rm p}$) used to compute the FT, the sampling interval ($\Delta t$), the mean amplitude in the FT ($\sigma$), the amplitude of the highest peak in the FT ($A_{\rm max}$), and a non-variability flag.} \end{table}