skip to content
 
Suzaku Guest Observer Facility

Updated XIS Calibration around 2 keV


In the Suzaku/XIS spectra of bright sources, residuals are often seen around 2 keV, with those in XIS1 (with the back-illuminated chip) being in the opposite sense to those in the other XIS units with front-illuminated chips.

The XIS team has released a set of new quantum efficiency files, dated 20120428.

  • This update modifies XAFS structures around the Si K edge and Al K edge by adopting new absorption coefficients.
  • The quantum efficiency of the BI CCD changes little (left) while those of FI CCDs change significantly (middle) to solve the "Si edge" problem.
  • X-ray transmission of the optical blocking filter around the Al K edge has also been updated (right).

Changes in QE Cal at 2 keV

The quantum efficiency files, ae_xiN_quanteff_20120428.fits (or later), are used by the RMF generator, xisrmfgen. To use the new calibration, install/use the latest calibration database and re-run xisrmfgen; there is no need to reprocess the event files or re-generate the ARF files.


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

This file was last modified on Friday, 08-Jun-2012 11:17:09 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: Phil Newman

    Privacy Policy and Important Notices.