![]() |
Figure 1: EPIC pn residuals around the iron line when no Gaussian lines are added to the model (see text for details). The energies are not corrected for the redshift of the source. |
Open with DEXTER |
![]() |
Figure 2: Best fit model and residuals for the pn/PDS spectrum (see text for details). |
Open with DEXTER |
![]() |
Figure 3:
![]() ![]() |
Open with DEXTER |
![]() |
Figure 4:
![]() ![]() |
Open with DEXTER |