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PIMMS Version 3.2a-d Release Notes
New and updated features in PIMMS v3.2a-d 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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