Choose the satellite carrying the instrument for which count rates are to be computed, a spectral model, and either flux or a reference comparison instrument. Then input these parameters.
This inteface to PIMMS has been adapted from W3PIMMS, a Web version of the PIMMS tool. PIMMS was developed by Koji Mukai at the HEASARC. The first Web version was developed at the SAX Data Center. The SAX PIMMS package was ported to and modified for the HEASARC Web site by Sherri Calvo. SXG PIMMS was adapted for the SXG Web site by Tomas P. Girnius.
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