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Background

  • We select one or two sources with a broad-band spectrum
  • Each of us contributes to the common exercise with:
    • Spectra and responses
    • A working hypothesis on a small number of calibration items which mostly affect the effective area
  • We fit together the astrophysics and the calibration working hypothesis
  • We evaluate whether the required modification to the calibration element makes sense
  • If not, we change the working hypothesis, and iterate
  • Please post proposed science cases as attachments and link them under the heading below (contact Eric Miller for help)
  • Comments on proposals can be added via the "Add Comment" box at the bottom of the page

Proposed Science Cases for Sources and Working Groups

3C273

Suzaku data: 

PKS2155

E0102

 


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