Figure 3.
The EPIC-pn and MOS2 observed data and the best-fitting const×tbabs×(diskbb+powerlaw) model (top panel) and residuals (bottom panel) for obs 1 (left) and obs 2 (right). The residuals show possible presence of emission features at ∼6.4 keV.

The EPIC-pn and MOS2 observed data and the best-fitting const×tbabs×(diskbb+powerlaw) model (top panel) and residuals (bottom panel) for obs 1 (left) and obs 2 (right). The residuals show possible presence of emission features at ∼6.4 keV.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close