...
- comparison of a celestial source
- E0102
- has been observed extensively over time with ACIS and XIS
- low energy lines very different from Mn K alpha
- mostly on ACIS-S3
- Perseus, other clusters
- check ACIS time coverage, XIS and ACIS roll angles
- Fe line centroid changes with kT, location in cluster
- E0102
Comments from MWB
- 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)