PIMMS Version 3.7/3.7a Release Notes

  • New in Version 3.7a (Released 2005 Nov 10; updated 2005 Dec 23)
    • The effective area curves for Chandra have been updated on Dec 23 (as Version 3.7a2) for AO-8 proposers (no code changes).
    • The effective area curves for the Suzaku XIS and HXD instruments have been updated.

  • New in Version 3.7 (Released 2005 Sep 13)
    • This version includes the AO-5 versions of XMM-Newton EPIC effective area curves, which differs slightly from the AO-4 versions. There are no updates for the RGS effective area.
    • This version also includes calibration updates of the RXTE PCA effective area curves. The count rate should increase by about 11% compared to previous versions. This is deemed minor enough that no impact is expected in proposal preparationss and in observation planning.
    • This version also includes post-launch calibration of the Swift XRT, in three data modes (photon counting, photodiode, and windowed timing).
    • PIMMS now uses the post-launch name, Suzaku, for the former Astro-E2.
    • This version now provides assumptions regarding the input count rate (such as extraction region for imaging instruments) for various missions.


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HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.

This file was last modified on Tuesday, 12-Sep-2006 14:45:52 EDT