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\begin{table*}
\parbox{15.6cm}{\caption[]{\label{liste02}X-ray sources detected in NGC~2516. 
Columns from left to right: 
running number,
sequence number, 
source coordinates  
RA (2\,000.0) and Dec (2\,000.0), both corrected for  pointing offset of 
$(+1\fs6, -4\farcs7)$, 
90\% confidence source radius $\Delta r$  in arcseconds, 
count rate in (ks)$^{-1}$, corrected for vignetting and for the 
life-time factor
( =0.978), 
hardness ratio HR1 and 
hardness ratio HR2.}}
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\begin{tabular}{rrrrllrrllcccc}
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\#$^{\rm a}$ & Seq$^{\rm b}$ &\multicolumn{3}{c}{RA  (2\,000.0)}  &\ & 
        \multicolumn{3}{c}{DEC (2\,000.0)} &\ & 
        $\Delta$\,r & 
        count rate & 
        HR1 & 
        HR2\\ 
 \cline{3-5}\cline{7-9}
  &   & (h) & (m)       & (s) &    &
       (\degr) & (\arcmin) &  (\arcsec) &  & 
       (\arcsec) &      
        (10$^{-3}$\,s$^{-1}$) & &  \\ 
\noalign{\smallskip}
\hline
\noalign{\smallskip}
 1& 61  & 07 & 52 & 35.3 & &-61 & 04 & 23.3 & &17.6   &  49$\pm$4 &  0.07$\pm$0.08 &  0.08$\pm$0.10 \\
 2& 35  & 07 & 52 & 53.5 & &-60 & 47 & 08.3 & &6.2    & 191$\pm$6 &  0.05$\pm$0.03 &  0.12$\pm$0.04 \\
 3& 45  & 07 & 55 & 02.45& &-60 & 49 & 13.4 & &15.6   & 8.7$\pm$1.4& 1.0$\pm$0.0 &  0.3$\pm$0.1\\
 4& 49  & 07 & 56 & 22.85& &-60 & 51 & 49.9 & &10.4   & 2.7$\pm$0.7& 1.0$\pm$0.0 &  0.2$\pm$0.3 \\
 5& 37  & 07 & 56 & 34.0 & &-60 & 48 & 04.5 & & 7.3   & 5.1$\pm$0.9& 1.0$\pm$0.07 & $-0.3\pm$0.2\\
 6& 32  & 07 & 56 & 38.4 & &-60 & 46 & 26.6 & &12.6   & 2.0$\pm$0.6& 1.0$\pm$0.0 &  0.8$\pm$0.2 \\
 7& 41  & 07 & 56 & 45.8 & &-60 & 48 & 53.5 & & 9.3   & 1.7$\pm$0.5& 1.0$\pm$0.0 &  0.65$\pm$0.25 \\
 8& 58  & 07 & 56 & 46.3 & &-60 & 56 & 50.5 & & 8.3   & 3.4$\pm$0.8& 1.0$\pm$0.0 & $-0.2\pm$0.2 \\
 9&  6  & 07 & 57 & 13.5 & &-60 & 33 & 13.4 & &12.5   & 3.8$\pm$0.9& 0.85$\pm$0.1 &  0.04$\pm$0.2 \\
10& 18  & 07 & 57 & 15.9 & &-60 & 41 & 00.9 & &13.2   & 2.6$\pm$0.7&  1.0$\pm$0.0 &  0.0$\pm$0.5\\
\\
11& 57  & 07 & 57 & 19.15 & &-60 & 56 & 34.0 & &12.3   &  1.9$\pm$0.6 &  1.0$\pm$0.1& $-0.35\pm$0.35\\
12& 60  & 07 & 57 & 19.95 & &-61 & 04 & 23.0 & &11.4   &  4.5$\pm$0.9 &  0.9$\pm$0.1 &  0.4$\pm$0.2\\
13& 39  & 07 & 57 & 20.6  & &-60 & 48 & 49.0 & &7.8    &  2.7$\pm$0.7 &  0.9$\pm$0.2 & $-0.1\pm$0.3\\
14& 46  & 07 & 57 & 23.8  & &-60 & 49 & 41.1 & &10.4   &  1.8$\pm$0.6 &  1.0$\pm$0.0 &   0.0$\pm$0.4\\
15& 14  & 07 & 57 & 27.7  & &-60 & 39 & 50.2 & &11.2   &  2.0$\pm$0.6 &  0.9$\pm$0.2&  0.6$\pm$0.3 \\
16& 48  & 07 & 57 & 28.25 & &-60 & 51 & 17.7 & & 9.4   &  1.5$\pm$0.5 &  1.0$\pm$0.0 &  0.1$\pm$0.5 \\
17& 59  & 07 & 57 & 31.6  & &-60 & 59 & 22.8 & & 8.5   &  3.0$\pm$0.7 &  1.0$\pm$0.0 &  0.0$\pm$0.25 \\
18& 12  & 07 & 57 & 31.95 & &-60 & 37 & 23.3 & &10.4   &  1.9$\pm$0.6 &  0.5$\pm$0.30&  0.65$\pm$0.3 \\
19& 54  & 07 & 57 & 38.0  & &-60 & 54 & 28.4 & & 8.3   &  1.9$\pm$0.6 &  1.0$\pm$0.0 & $-0.1\pm$0.3\\
20&  1  & 07 & 57 & 49.95 & &-60 & 17 & 59.0 & &18.3   & 15.3$\pm$2.0 & $-0.99\pm$0.07 & $-1.0\pm$0.0\\
\\
21& 63  & 07 & 57 & 53.9 & &-61 & 19 & 19.1 & &29.7    & 6.4$\pm$1.5 &  0.65$\pm$0.2 &  0.3$\pm$0.2 \\
22&  9  & 07 & 57 & 55.1 & &-60 & 36 & 00.6 & & 8.3    & 2.6$\pm$0.7 &  0.9$\pm$0.2 &  0.2$\pm$0.3 \\
23& 17  & 07 & 57 & 55.15& &-60 & 40 & 39.1 & & 8.3    & 2.3$\pm$0.6 &  1.0$\pm$0.0 &  0.1$\pm$0.3 \\
24& 38  & 07 & 57 & 55.6 & &-60 & 48 & 28.6 & & 5.5    & 3.2$\pm$0.7 &  1.0$\pm$0.1 &  0.0$\pm$0.2 \\
25& 51  & 07 & 57 & 59.6 & &-60 & 52 & 29.1 & & 8.6    & 3.3$\pm$0.7 &  0.7$\pm$0.2 & $-0.9\pm$0.1 \\
26& 33  & 07 & 58 & 02.55& &-60 & 46 & 49.6 & & 6.1    & 2.8$\pm$0.6 &  1.0$\pm$0.0 & $-0.55\pm$0.2 \\
27& --- & 07 & 58 & 03.1 & &-60 & 48 & 49.2 & & 9.9    & 1.4$\pm$0.5 &  1.0:            & $-0.4:$  \\
28& 10  & 07 & 58 & 05.9 & &-60 & 35 & 57.1 & & 4.1    &11.9$\pm$1.3 &  0.22$\pm$0.11 & $-0.06\pm$0.13\\
29& 27  & 07 & 58 & 07.3 & &-60 & 44 & 49.6 & &10.6    & 2.7$\pm$0.7 &  1.0$\pm$0.0 &  1.0$\pm$0.0 \\
30&  2  & 07 & 58 & 09.4 & &-60 & 21 & 54.1 & & 21.3    &  4.9$\pm$1.2 &  0.4$\pm$0.25 & 0.0$\pm$0.25\\
\\
31& 50  & 07 & 58 & 10.3 & &-60 & 51 & 55.6 & &  6.8    &  2.4$\pm$0.6 &  1.0$\pm$0.0 &  0.6$\pm$0.3 \\
32&  8  & 07 & 58 & 16.5 & &-60 & 35 & 52.1 & & 7.6    & 2.7$\pm$0.8 &  0.3$\pm$0.1 &  0.0$\pm$0.1 \\
33& 28  & 07 & 58 & 18.3 & &-60 & 45 & 16.6 & & 7.6     &  2.1$\pm$0.6 &  1.0$\pm$0.0 & $-0.2\pm$0.25 \\
34& --- & 07 & 58 & 22.0 & &-60 & 51 & 29.6 & & 8.1     &  1.5$\pm$0.5  &       1.0:     &          0.1:\\
35& 55  & 07 & 58 & 22.8 & &-60 & 54 & 58.6 & & 5.0     &  4.8$\pm$0.8 &  0.9$\pm$0.1 &  0.1$\pm$0.2 \\
36&15   & 07 & 58 & 23.2 & &-60 & 40 & 25.6 & & 5.6     &  3.7$\pm$0.7  &  1.0$\pm$0.0 & $-0.2\pm$0.2 \\
37& 43  & 07 & 58 & 30.5 & &-60 & 49 & 05.5 & &  9.3    &  1.7$\pm$0.5 &  1.0$\pm$0.0 & $-1.0\pm$0.0 \\
38& 20  & 07 & 58 & 30.65& &-60 & 41 & 57.0 & & 8.5     &  2.0$\pm$0.6 &  1.0$\pm$0.0 &  0.3$\pm$0.3 \\
39& 30  & 07 & 58 & 31.85& &-60 & 46 & 03.5 & & 6.5     &  3.3$\pm$0.7 &  1.0$\pm$0.0 & $-0.1\pm$0.3 \\
40& 25  & 07 & 58 & 33.6 & &-60 & 44 & 29.5 & & 5.9     &  3.8$\pm$0.7 &  1.0$\pm$0.0 & $-0.7\pm$0.2 \\
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\end{tabular}
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\end{table*}
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\begin{table*}
\caption[]{(continued)}
\begin{flushleft}
\begin{tabular}{rrrrllrrllcccc}
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\hline
\noalign{\smallskip}
\#$^{\rm a)}$ & Seq$^{\rm b)}$ &\multicolumn{3}{c}{RA  (2\,000.0)}  &\ & 
        \multicolumn{3}{c}{DEC (2\,000.0)} &\ & 
        $\Delta$\,r & 
        count rate & 
        HR1 & 
        HR2\\ 
 \cline{3-5}\cline{7-9}
  &   & (h) & (m)       & (s) &    &
       (\degr) & (\arcmin) &  (\arcsec) &  & 
       (\arcsec) &      
        (10$^{-3}$\,s$^{-1}$) & &  \\ 
\noalign{\smallskip}
\hline
\noalign{\smallskip}
41& 34  & 07 & 58 & 35.7 & &-60 & 46 & 54.5 & & 5.8     & 3.1$\pm$0.7 &  0.7$\pm$0.2   & $-0.1\pm0.2$  \\
42& 47  & 07 & 58 & 36.6 & &-60 & 50 & 22.5 & & 6.2     & 2.3$\pm$0.6 &  1.0$\pm$0.0 & 0.1$\pm$0.3 \\
43& 19  & 07 & 58 & 40.5 & &-60 & 41 & 44.4 & & 6.5     & 3.0$\pm$0.7 &  1.0$\pm$0.0 &  0.8$\pm$0.2 \\
44& 56  & 07 & 58 & 42.8 & &-60 & 55 & 26.9 & & 5.8     & 4.2$\pm$0.8 &  1.0$\pm$0.05 &  0.4$\pm$0.15\\
45& 52  & 07 & 58 & 49.35& &-60 & 54 & 10.8 & & 6.7     & 5.4$\pm$0.9 &  0.75$\pm$0.15 & $-0.15\pm0.2$ \\
46& 44  & 07 & 58 & 50.3 & &-60 & 49 & 29.2 & & 3.9     & 6.1$\pm$0.9 &  1.0$\pm$0.0 &  0.2$\pm$0.15\\
47& 13  & 07 & 58 & 50.65& &-60 & 38 & 40.2 & & 2.9     &14.5$\pm$1.4 &  0.98$\pm$0.03&  0.19$\pm$0.10\\
48& 11  & 07 & 58 & 53.45& &-60 & 35 & 59.2 & & 9.2     & 4.3$\pm$0.9 &  0.96$\pm$0.07 &  0.0$\pm$0.2\\
49&  4  & 07 & 58 & 54.9 & &-60 & 30 & 15.7 & &13.8     & 3.2$\pm$0.8 &  0.9 $\pm$0.1  &  0.1 $\pm$0.2\\
50& 23  & 07 & 58 & 57.75& &-60 & 43 & 02.6 & & 6.6     & 2.9$\pm$0.7 &  1.0$\pm$0.0 &  0.0 $\pm$0.3\\
\\
51& 29  & 07 & 59 & 20.15& &-60 & 45 & 32.5 & & 6.2     &  3.5$\pm$0.7 &  0.94$\pm$0.07 &  0.0$\pm$0.2\\
52& 42  & 07 & 59 & 20.4 & &-60 & 48 & 56.5 & & 5.9     &  3.2$\pm$0.7 &  1.0$\pm$0.0 &  0.3 $\pm$0.3\\
53& 36a & 07 & 59 & 23.8 & &-60 & 47 & 34.9 & & 11.1    &  2.5$\pm$1   &  0.9$\pm$0.1 &  0.75$\pm$0.1\\
54& 36b & 07 & 59 & 28.3 & &-60 & 47 & 45.3 & & 15:     &  1.8$\pm$0.6 & 0.9$\pm$0.2    & 0.8$\pm$0.2  \\
55& 40  & 07 & 59 & 31.9 & &-60 & 48 & 50.1 & & 6.9     &  3.0$\pm$0.7 & 1.0$\pm$0.0 & $-0.3\pm0.2$ \\
56& 26  & 07 & 59 & 33.1 & &-60 & 44 & 34.9 & & 7.0     &  3.3$\pm$0.7 &  0.8$\pm$0.2 &  0.05$\pm$0.2\\
57& 22  & 07 & 59 & 39.95& &-60 & 42 & 37.7 & & 10.5   &   1.8$\pm$0.6 &  1.0$\pm$0.0 & -0.4$\pm$0.3\\
58& 24  & 07 & 59 & 50.55& &-60 & 43 & 30.3 & & 9.2    &   2.7$\pm$0.7 &  0.9$\pm$0.1   &  0.5$\pm$0.2\\
59&  3  & 08 & 0 & 0.85  & &-60 & 23 & 33.2 & &27.6     &  5.2$\pm$1.2 &  0.6$\pm$0.2 &  0.0$\pm$0.2\\
60& 53  & 08 & 0 & 13.4  & &-60 & 53 & 09.6 & &12.0     &  2.0$\pm$0.6 &  0.8$\pm$0.2   &  0.5$\pm$0.2\\
\\
61& 62  & 08 & 0 & 17.3 & &-61 & 09 & 50.4 & & 6.8      & 31.7$\pm$2.3 &  0.10$\pm$0.07  &  0.01$\pm$0.09\\
62& 21  & 08 & 0 & 23.8 & &-60 & 42 & 03.5 & & 8.6     &  12.8$\pm$1.5 &  0.97$\pm$0.03 &  0.26$\pm$0.10\\
63&  5  & 08 & 0 & 56.45 & &-60 & 31 & 08.2 & & 19.7    &  5.9$\pm$1.3 &  0.5$\pm$0.25 & $-0.05\pm0.25$ \\
64&  7  & 08 & 02 & 22.3  & &-60 & 34 & 29.8 & &18.3    & 23.0$\pm$2.5 &  1.0$\pm$0.0 & 0.25$\pm$0.1\\
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\end{tabular}
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Notes:\\
a) running number (increasing with $\alpha$)\\
b) X-ray source number, as detected with {\it EXSAS}  reduction package
(increasing with $-\delta$)\\
\end{table*}
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