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There are several quantities used in the simulators that must be tuned
in order to get the simulations to reproduce adequately the XRCF PSF data.
- Focus - can be adjusted to match the data fairly well just by
examining the rays (we used the ``dataset_2d'' tool, part of
the TARA package, and the MARX output files ``xpixel.dat'' and
``ypixel.dat''), since this parameter is controlled by MARX.
- Flux - tuning the flux is crucial for reproducing XRCF data,
since this is the way to reproduce and explore pile-up. The
current analysis suffers from a lack of flux tuning capability,
but this will hopefully be available in the next MARX release. For
now, we have forced the simulator to the idealized state of
exactly one photon per frame.
- FAM orientation (CHIPX & CHIPY offsets, rotation) - we have
implemented the ability to adjust the position of the PSF
in CHIPX and CHIPY, but have not yet explored the possibility of
rotation.
- Others? - As we tune the above parameters and improve the
simulator, we may discover other parameters whose tuning
allows us to reproduce the data more accurately. We remain
alert for such potential adjustments.
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Up: ACIS/HRMA Point Spread Function
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Please address comments and questions to Dr. John Nousek ( nousek@astro.psu.edu )