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1. Introduction
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Suzaku Technical Description
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List of Figures
Contents
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
) to cause the indicated pile-up fraction as a
function of PSF radius.
)a