\begin{table}%t1
\caption{\label{tbl:werte2}IPs detected in the BAT survey  3$\sigma$ in the 15$-$55~keV band ordered by constellation. The first three columns give the BAT~position and the offset to the optical position. The count rate  was averaged over the entire 2.5~yr  observing period. In the lower part of the table we report those sources which are not currently detected in the BAT~survey; for those we give the optical position for which the upper limit was computed.}
\small%\centerline
 {
\begin{tabular}{lrrrcrcc}
\hline 
\hline 
%&&&&&&& \\[-8pt]
   \textbf{Name} & RA & Dec & Offset & Count rate~~~ & Significance & Exp. time & Sensitivity$^1$\\
         & (2000.0) & (2000.0) & (arcmin) & (10$^{-5}$  cts/s/det) & ratio & (Ms) & (10$^{-11}$ erg/cm$^2$/s) \\
 \hline 
 FO Aquarii          & 334.481 & --8.351 &3.3 &12.4 $\pm$ 0.8  & 16.6& 2.76 & 1.99 \\
 XY Arietis          & 44.038  & 19.441 &4.3 & 5.3 $\pm$ 0.6  & 7.9 & 2.70 & 1.55 \\
 V405 Aurigae        & 89.497  & 53.896 &0.3 & 5.4 $\pm$ 0.6  & 8.7 & 2.70 & 1.66 \\
 MU Camelopardaris   & 96.318  & 73.578 &1.4 & 2.9 $\pm$ 0.5  & 6.7 & 3.46 & 1.60 \\
 V709 Cassiopeiae    & 7.204   & 59.289 &0.7 &16.2 $\pm$ 0.7  & 27.5& 3.65 & 1.61 \\
 V1025 Centauri      & 189.569 & --38.713&4.1 & 1.6 $\pm$ 0.8  & 3.1 & 1.91 & 1.88 \\
 BG Canis Minoris    & 112.871 & 9.940  &2.9 & 5.8 $\pm$ 0.8  & 7.0 & 1.92 & 2.15 \\
 TV Columbae         & 82.356  & --32.818&2.5 &13.0 $\pm$ 0.7  & 20.3& 3.55 & 1.44 \\
 TX Columbae         & 85.834  & --41.032&3.5 & 4.5 $\pm$ 0.5  & 7.8 & 3.81 & 1.31 \\
 V2306 Cygni         & 299.560 & 32.545 &3.4 & 3.1 $\pm$ 0.5  & 4.8 & 3.85 & 1.77 \\
 DO Draconis         & 175.910 & 71.689 &1.8 & 2.7 $\pm$ 0.4  & 7.8 & 4.47 & 1.11 \\
 PQ Geminorum        & 117.822 & 14.740 &2.7 & 6.2 $\pm$ 0.7  & 9.4 & 2.04 & 2.17 \\
 EX Hydrae           & 193.102 & --29.249&3.0 & 5.2 $\pm$ 0.7  & 6.4 & 1.87 & 1.97 \\
 NY Lupi             & 237.061 & --45.478&2.1 &15.2 $\pm$ 0.8  & 15.5& 1.35 & 2.58 \\
 V2400 Ophiuchi      & 258.152 & --24.246&4.2 &10.5 $\pm$ 0.9  & 11.0& 1.30 & 2.52 \\
 GK Persei           & 52.799  & 43.905 &4.4 &18.5 $\pm$ 0.9  & 30.4& 2.88 & 1.58 \\
 AO Piscium          & 343.825 & --3.178 &4.7 & 8.1 $\pm$ 0.6  & 11.1& 3.00 & 1.62 \\
 V1223 Sagittarii    & 283.759 & --31.163&3.0 &19.6 $\pm$ 1.1  & 20.8& 1.31 & 2.54 \\
 V1062 Tauri         & 75.615  & 24.756 &5.3 & 3.1 $\pm$ 0.8  & 5.9 & 2.09 & 2.25\\
 RX J2133.7+5107     & 323.432 & 51.124 &1.9 &10.9 $\pm$ 0.6  & 18.2& 3.99 & 1.42 \\
 Swift J0732.5-1331  & 113.156 & --13.518&2.8 & 6.3 $\pm$ 0.6  & 9.7 & 2.61 & 1.70 \\
 IGR J00234+6141     & 5.740   & 61.686 &5.3 & 2.0 $\pm$ 0.6  & 3.0 & 3.68 & 1.72 \\
 IGR J17303-0601     & 262.590 & --5.993 &0.8 &14.0 $\pm$ 0.8  & 12.7& 1.59 & 2.78\\
 \hline
 AE Aquarii          & 310.04 & --0.87 & --&$<$$0.3$ & 0.4& 2.44 & 2.05\\
 HT Camelopardaris   & 119.26 & 63.10 & --&$<$$0.1$ & 0.3 & 3.52 & 1.34 \\
 DW Cancri           & 119.72 & 16.28 & --&$<$$1.5$ & 1.5 & 2.09 & 2.11 \\
 UU Columbae         & 78.05  & --32.69& --&$<$$0.7$ & 1.7 & 3.55 & 1.50 \\
 DQ Herculis         & 271.88 & --45.86& --&$<$$1.0$ & 2.5 & 3.75 & 1.56 \\
 WX Pyxidis          & 128.27 & --22.81& --&$<$$1.4$ & 2.8 & 3.16 & 1.56\\
 \hline 
 \end{tabular}}
\medskip
$^1$ Minimum flux to detect a source at 3$\sigma$ at a given position in the 15$-$55~keV band.
\end{table}