\begin{table}%T4
\caption{This table lists the maximum detection significance reached during the
hexagonal dither observations (Sig$_{\rm rev,~max}$), the detection significance per season (Sig$_{\rm sX}$; where $X=1$,~2,~3 
for the three seasons) and the detection significance for all observations together (Sig$_{\rm all}$), together 
with the corresponding fluxes ($F_{\rm sX}$) and errors in the fluxes for the 
IBIS/ISGRI 60$-$150~keV band. The ordering of sources is the same as used for Table~1.
We only list those sources for which either Sig$_{\rm rev,~max}$, Sig$_{\rm sX}$ or Sig$_{\rm all}$ reached a value higher
than~7. When a source was not detected it is indicated with "$-$''; we then provide a 3$\sigma$ (statistical) upper limit
on the flux. Whenever Sig$_{\rm rev, max}$ exceeds 7, the source long-term light curves are discussed in Sect.~\ref{light_curves}.
}
\label{significance_2}
\small%%\centering

\par
\begin{tabular}{l|ccccccccc}
\hline\hline
\multicolumn{1}{l|}{} &
\multicolumn{1}{c}{Sig$_{\rm rev,~max}$} &
\multicolumn{1}{c}{Sig$_{\rm s1}$} &
\multicolumn{1}{c}{$F_{\rm s1}$} &
\multicolumn{1}{c}{Sig$_{\rm s2}$} &
\multicolumn{1}{c}{$F_{\rm s2}$} &
\multicolumn{1}{c}{Sig$_{\rm s3}$} &
\multicolumn{1}{c}{$F_{\rm s3}$} &
\multicolumn{1}{c}{Sig$_{\rm all}$} &
\multicolumn{1}{c}{$F_{\rm all}$} \\
\multicolumn{1}{l|}{Source} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{(mCrab)} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{(mCrab)} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{(mCrab)} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{(mCrab)} \\
\hline
GS~1826$-$24       & 11.0 & 29.5 & 12.2 $\pm$ 0.4 &  33.7 & 13.4 $\pm$ 0.4 & 30.2 & 12.2 $\pm$ 0.4 &  53.6 & 12.8 $\pm$ 0.2 \\
GRS~1758$-$258     & 28.9 & 95.3 & 23.8 $\pm$ 0.2 & 103.4 & 26.2 $\pm$ 0.2 & 79.5 & 19.5 $\pm$ 0.2 & 161.3 & 23.2 $\pm$ 0.1 \\
GX~1+4             &  9.3 & 14.1 &  3.7 $\pm$ 0.2 &  18.1 &  4.9 $\pm$ 0.2 & 23.3 &  6.1 $\pm$ 0.2 &  31.8 &  4.9 $\pm$ 0.1 \\
XB~1832$-$330      &  4.3 &  6.2 &  3.0 $\pm$ 0.4 &   4.1 &  1.8 $\pm$ 0.4 &  8.0 &  3.7 $\pm$ 0.4 &  10.2 &  2.4 $\pm$ 0.2 \\
SLX~1735$-$269     &  5.2 & 10.0 &  2.4 $\pm$ 0.2 &   9.8 &  2.4 $\pm$ 0.2 & 10.0 &  2.4 $\pm$ 0.2 &  16.7 &  2.4 $\pm$ 0.1 \\
XTE~J1817$-$330    & 11.1 &  $-$ & $<$3.4         &   $-$ & $<$3.4         & 22.1 &  6.7 $\pm$ 0.3 &  12.6 &  2.4 $\pm$ 0.2 \\
1A~1742$-$294      &  5.0 &  6.1 &  1.2 $\pm$ 0.2 &   $-$ & $<$2.8         &  9.4 &  2.4 $\pm$ 0.2 &   7.6 &  1.2 $\pm$ 0.2 \\
SLX~1744$-$299/300 &  4.4 &  $-$ & $<$2.7         &   6.7 &  1.8 $\pm$ 0.2 &  5.4 &  1.2 $\pm$ 0.2 &   8.2 &  1.2 $\pm$ 0.1 \\
1E~1740.7$-$2942   & 19.8 & 58.8 & 14.0 $\pm$ 0.2 &  50.1 & 11.6 $\pm$ 0.2 &  $-$ & $<$2.7         &  61.9 &  8.5 $\pm$ 0.1 \\
H1743$-$322         & 13.2 &  $-$ & $<$2.7         &  15.4 &  3.7 $\pm$ 0.2 &  $-$ & $<$2.8         &   9.6 &  1.2 $\pm$ 0.1 \\
4U~1722$-$30       &  5.4 & 11.7 &  3.0 $\pm$ 0.2 &   7.1 &  1.8 $\pm$ 0.2 &  6.9 &  1.8 $\pm$ 0.2 &  15.2 &  2.4 $\pm$ 0.1 \\
IGR~J17098$-$3628  & 10.0 &  $-$ & $<$4.2         &  $-$  & $<$4.5         &  $-$ & $<$4.3         &  $-$  & $<$2.5         \\
4U~1700$-$377      & 33.7 & 48.0 & 22.0 $\pm$ 0.4 &  40.0 & 19.5 $\pm$ 0.5 & 28.4 & 13.4 $\pm$ 0.5 &  67.7 & 18.3 $\pm$ 0.2 \\
GRO~J1655$-$40     & 21.4 & 23.0 & 17.1 $\pm$ 0.7 &   9.4 &  7.3 $\pm$ 0.8 &  $-$ & $<$8.7         &  18.6 &  7.9 $\pm$ 0.4 \\
\hline
\end{tabular}
\end{table}