 |
Figure 1:
Light curves of NGC 3226 obtained with the EPIC p-n ( left)
and the EPIC MOS ( right) cameras in the 0.3-10 keV band. The events
are binned into 900 s time intervals. The error bars give the 1
count rate errors of each individual bin. |
| Open with DEXTER | |
In the text
 |
Figure 2:
Left: simultaneous fit (see Table 2) of the EPIC pn, EPIC
MOS 1 and EPIC MOS 2 spectra by a bremsstrahlung model absorbed by
neutral gas. The 
distribution is displayed
in the lower panel. The corresponding spectral model (bold line) is
plotted on the right panel and compared with the best fit absorbed
power law model (dashed line) described in Table 2 (Model B). |
| Open with DEXTER | |
In the text