Table 6: Summary of of our sample of pointings performed with XMM-Newton (see also Table 3). The directions of the pointings have been specifically selected to study the contribution of the SXRB as seen by XMM-Newton.
Observation ID Galactic  coordinates $N_{\mbox{{\scriptsize H {\sc i}}}}$ ${t_{\rm total} ~\rm [ks]}$ $t_{\rm effective} ~\rm [ks]$
        l [$^\circ$]       b [$^\circ$] [1020 cm-2] MOS pn MOS1 MOS2 pn

0110660301

     125.0554     30.5087 8.2 8.9 5.2 5.4 5.7 2.9
0110660401     165.1789     66.5823 3.3 13.2 9.3 11.1 10.9 6.0
01106606012     95.0340     38.9844 2.6 16.1 12.4 12.0 13.6 12.2
01106608012     91.3173     37.0343 2.3 12.2 9.2 10.3 10.4 9.2
01106616012     125.0554     30.5087 8.2 10.0 6.0 10.0 10.0 6.0
01106617012     153.2919     39.3394 6.4 11.2 11.6 9.7 11.2 11.6
01106624012     87.9566     36.3392 2.5 8.7 5.6 8.7 8.7 5.6
01106626012     90.8139     37.9770 1.7 11.4 8.0 10.1 9.8 8.0
01106627012     88.9394     37.1270 1.9 9.7 6.3 7.9 8.0 4.9
2 Like in Table 3.


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 XMM-Newton raw and calibrated data
3 Data reduction
4 Exposure maps
5 Radial asymmetry of the XMM-Newton EPIC MOS1 vignetting in the soft energy regime
6 Conclusions
References
Online Material
List of tables
List of figures