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PIMMS Version 3.4/3.4a Release Notes
New and updated features in PIMMS v3.4/3.4a are:
- V3.4a
includes updated Chandra effective area curves, appropriate for
Cycle 6
proposals (these files are available in
chandra-ao6.tar.gz). Those who wish to convert count
rates in past observations to flux, please see this
note.
- Swift effective
area curves are included. To enable UVOT count rate predictions,
a new UV/optical extinction function has been added to the
code
UK mirror maintained
by: Dr. Duncan Law-Green, LEDAS Support Scientist
(dlg@star.le.ac.uk), (0116)
252-2589.
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