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A count rate of 4000 counts per second per two cameras corresponds
to 1 Crab. Typically, the charge cloud produced by an X-ray photon is
not localized to one pixel but spread out over several pixels. There
are two data modes, ``faint" and ``bright", which correspond to two
different ways of telemetering this spread to the ground within the
available data rate.
- Faint mode: SIS spectra in this mode have 4096 channels.
The pixel position of the center of the event is given, along with the
pulse height recorded in the nine pixels around it (central pixel plus
eight surrounding pixels in a 3 x 3 grid).
- Bright mode: SIS spectra in this mode have 2048 channels.
The pixel position of the center of the event is given, together with
the ``grade" describing the nature of the spread, and the total pulse
height above an adjustable threshold.
Additional, primarily diagnostic modes also exist. Verification of all
modes is the responsibility of ISAS, the Astro-D GOF and the
Pennsylvania State University.
In 4-CCD mode, at high bit-rate, the maximum count rates are 32 and
128 counts per second per two cameras in faint and bright modes,
respectively. In 1-CCD mode, these figures are four times larger.
Next: GIS
Up: SIS
Previous: CCD clocking modes
Keith Arnaud
1/5/1998