skip to content
 
Suzaku Guest Observer Facility

The Accuracy of HXD/PIN Response


The response matrices of HXD/PIN have been verified using the Crab observations, for both of the XIS-nominal and HXD-nominal pointing positions. Results are shown in below (see also the PDF version). Discrepancies between the data and model are smaller than a few percent in the energy range of 12-40 keV.

XIS nominal HXD nominal


If you have any questions concerning Suzaku, visit the Feedback form.

This file was last modified on Friday, 15-Sep-2006 19:09:42 EDT

NASA Astrophysics

  • FAQ/Comments/Feedback
  • Education Resources
  • Download Adobe Acrobat
  • A service of the Astrophysics Science Division (ASD) at NASA/ GSFC

    Suzaku Project Scientist: Dr. Robert Petre
    Responsible NASA Official: Dr. Andy Ptak

    Privacy Policy and Important Notices.