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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.
7.1.
Effective area and exposure time for different Burst and Window options.
7.2.
Journal of SCI operations.
7.4.
Major XIS Background Emission Lines (Tawa et al. 2008).
7.5.
Supported clock modes and options with the SCI.
7.6.
Total count rate which causes the indicated fraction of pile-up in a circle with the indicated radius range.
7.7.
Telemetry allocation (kbit/s).
7.8.
Typical event size after compression [byte].
7.9.
Maximum counting rates for avoiding telemetry saturation [counts/s/XIS].
7.10.
Maximum counting rate for avoiding pile-up.
7.11.
Relative normalization between different sensors.
Michael Arida 2011-10-06