\begin{table}%t1
%\centering
\par
\caption{\label{tabpos}IBIS/ISGRI best-fit positions of the Crab in 3 energy bands. }
\small 
\begin{tabular}{lcccc}
\hline\hline\noalign{\smallskip}
~ & RA [$^\circ$] & Dec [$^\circ$] & $\sigma_{\mbox{\tiny{stat+syst}}}$ [$''$] & Shift [$''$]\\
\hline
Total, 20--40~keV & 83.6317 & 22.0162 & 0.6 & 8.0\\
Total, 40--100~keV & 83.6319 & 22.0159 & 0.7 & 6.7\\
Total, 100--200~keV & 83.6321 & 22.0157 & 1.0 & 5.8\\
Off-pulse, 20--40~keV & 83.6315 & 22.0164 & 0.7 & 9.0\\
On-pulse, 20--40~keV & 83.6319 & 22.0160 & 0.7 & 7.0\\
Off-pulse, 40--100~keV & 83.6316 & 22.0161 & 0.8 & 8.0\\
On-pulse, 40--100~keV & 83.6322 & 22.0158 & 0.7 & 5.9\\
Off-pulse, 100--200~keV & 83.6316 & 22.0162 & 1.2 & 8.2\\
On-pulse, 100--200~keV & 83.6323 & 22.0155 & 1.1 & 4.8\\
\hline 
\end{tabular}
\smallskip 
The phase-resolved positions (on- and off- pulse) are also reported. The $1\sigma$ error on the position (3rd~column) is the sum of the statistical and systematic uncertainties, where the systematic error is fixed to be 0.5$''$ (see Sect.~\ref{syst}). The last column gives the angular distance between the measured position and the pulsar (in arcsec).
\end{table}