Image 3: Model spectrum after filtering on energy
![[Image 3: Model spectrum after filtering on energy]](energy_ranges.gif)
The red and green lines show the source spectrum after filtering on the rest- and observed-frame energy ranges (they have been offset from each other by 20 per cent for clarity).
The model used here is the XSMEKAL plasma model with a temperature of 7 keV, metallicity abundance of 0.3 times solar, and a redshift of 0. The observed energy range is taken to be 0.5-2.0 keV and the source redshift (for calculating the rest-frame energy range) is 0.4.
