Subject: JEMX Monday Meeting 2004-10-04 Present: CAO, SB, ILR, NL, JC, CBJ, NJW JEMX status: After onset of JMX2 it takes about 5 hours for gain stabilization. This has implications for the recent Crab calibrations where the first measurements are somewhat disturbed by this continuing gain increase. JC: The Xe line position in energy (measured by PI value) is slowly increasing with time. This probably means that the gain under the FRSS sources is decreasing. CAO will introduce a time dependent correction factor for the OSA5 delivery of j_cor_gain. CBJ: The weighted average of Kalpha1(2) and Kalpha2(1) line position from table is 29.696 keV for Xe. JC will try to find the Mo line (at 17.4 keV) to see if its time dependence is similar to the Xe line, but this can be tricky and will take some time. The aim is to see if gas deterioration or local gain decrease is the cause. For the next Crab calibration we should change the cathode voltage (VC) with a factor 1.5 (about the limit). If the gas is OK there should be no change of Xe peak position JMX2 has not shown any degradation while dormant. Crab calibration: The measured flux changes with position in the FOV which is a concern. A tilted collimator can explain some but not all of these variations. Work is continuing. ISWT meeting: Dither pattern will be changed so that consequtive cycles will not be identical (roll angle change by +-3 deg) Unused TOO time of the core program will be used for ironing out the GPS coverage and saved for later (fifty-fifty). Data analysis: Perseus and SGR1806 are analyzed. /NJW ---------- Niels J. Westergaard Danish Space Research Institute Juliane Maries Vej 30, DK 2100 Copenhagen O Phone: +45 35 32 57 05; FAX: +45 35 36 24 75