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The average pulse profile consists of two peaks of similar size
separated by
. Figure 3.3
shows the folded intensity and hardness profiles for different orbital
phases. The factor of
four change in the X-ray intensity through the observation is accompanied
by significant changes in the pulse profile.
The profile also has different energy dependence at different orbital
phases.
Figure 5:
Orbital phase resolved GIS pulse profiles and hardness ratios. The
upper panel is the 0.7-11 keV intensity divided by the pulse-phase average.
The lower panel is the ratio of the 0.7-4.5 keV count rate to the
4.5-11 keV count rate.
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Damian Audley
1998-09-04