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  • outline quite broad, might want to focus it more
  • (his) primary goal: understand the relationship between spectral resolution, radiation damage, and background
    • frame-to-frame variations in BG lead to variations in trap filling and wobbling of LSF
    • Suzaku especially good since we can already model the BG as a function of orbital position
  • secondary goal: construct a model of the background
    • test this model with a simulated BG (e.g. from Co60 source) in the lab (perhaps follow-up paper)

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