Table A.1:
M 83 sources detected at the 3-
level
in the 0.3-8.0 keV band, and respective net fluxes in a soft, medium and hard band.
Counts in a given band are given in brackets when the source was detected
at less than 3- level in that band. The exposure time was 50.851 ks.
The ROSAT cross-identification refers to the HRI sources listed by Immler et al. (1999);
SW02 is the cross-identification with Soria & Wu (2002).
![\begin{table}
\par
\begin{displaymath}
\begin{array}[width=textwidth]{rcccrrrr...
...& (1.7\pm1.7) & (^{{b}}) & 33\\
\hline
\end{array}\end{displaymath}\end{table}](/articles/aa/full/2003/40/aah4147/img155.gif)
![\begin{table}\begin{displaymath}
\begin{array}[width=textwidth]{rcccrrrrrr}
\h...
...3\pm03.0 & (0.5\pm0.5)& & 72\\
\hline
\end{array}\end{displaymath}\end{table}](/articles/aa/full/2003/40/aah4147/img156.gif)
![\begin{table}\begin{displaymath}
\begin{array}[width=textwidth]{rcccrrrrrr}
\h...
...ray source coincident with the IR/optical/UV nucleus of the galaxy.
\end{table}](/articles/aa/full/2003/40/aah4147/img157.gif)
level
in the 0.3-8.0 keV band, and respective net fluxes in a soft, medium and hard band.
Counts in a given band are given in brackets when the source was detected
at less than 3-