This webpage provides a discussion of cross-calibration work
relating the Chandra X-ray Observatory to other X-ray
missions, particularly XMM-Newton. Much of this webpage was
developed in cooperation with the
XMM-Newton calibration team.
If new calibration has been applied to the event file, the
grating spectrum should be re-extracted as well. It is then
possible to build grating response files (gARF, gRMF) in order
to model and fit the data in Sherpa.