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List of Tables
- 3.1. Overview of Suzaku capabilities.
- 3.2. Error Budgets of Scientific Instrument Calibrations.
- 4.1. Suzaku time allocated to each group of observers. The ESA time is in parentheses as it is part of the Japanese allotment.
- 6.1. Telescope dimensions and parameters of XRT-I.
- 6.2. Design parameters for the pre-collimator.
- 6.3. Best-fit parameters of the power law model fits to the Crab spectra taken on 2005 September 15-16.
- 6.4. Best-fit parameters of the contemporaneous power-law fits to the Crab spectra taken in 2005 September 15-16.
- 7.2. Clocking modes
- 7.3. Window and burst options (XIS nominal position)
- 7.4. Editing modes and size per event for observation modes
- 7.5. Combination of editing modes and PPU ratio
- 7.6. Event threshold
- 7.7. Total count rate (s) to cause the indicated pile-up fraction as a function of PSF radius.
- 7.8. Telemetry allocation for XIS
- . Incoming rate to cause telemetry saturation (s)a
- 7.11. Strength of emission lines in the NXB spectrum
- 7.12. Relative normalization among different sensors.
Michael Arida 2012-10-19