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Instructions

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

Current Proposals/White Papers for Sources and Working Groups




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