Subject: JEM-X Monday Meeting 2007-12-10 Date: Mon, 10 Dec 2007 14:05:55 +0100 (MET) Participants: SB, NL, JC, CBJ, CAO, NJW. JEM-X status (SB): Nothing to report. No hotspot activity. Some radiation at the end of each revolution. INTEGRAL shifts the nominal radiation belt to a larger altitude. For the TM there is a safety buffer that currently is not exploited. An overbooking in the polling cycle will provoke some use of the extra buffer. Consequently a few extra packets can be transmitted. This has been run on the simulator and will probably be tested on the spacecraft soon. Calibration (SB): The public data up to revolution 496 has been used to generate a new SPAG (spatial gain map). 6 epochs, each with about 50 revolutions, have been used. The work is ongoing. A plot of the Xe line per anode (given RAWX value) is an auxiliary indicator of the degree of life in an anode strip. The long integration time can also reveal more details of anodes that are not interrupted at their root but at some distance from it. Crab calibration (SB, CBJ): The goal is to reach an absolute assessment of the Crab intensity. A selection of the best area of the detector where there is little doubt of the efficiency (i.e. no loss in weak anodes). j_ima_iros status (NL): Systematic effects: - The derived flux changes from one Crab calibration period to the next It is not clear why this is so. The cause can be outside OSA. There is a step after revol. 45. We must check if there is a change of a setting of .e.g. a discriminator. - Radius dependence - Azimuth dependence We must make at least one IMOD epoch per Crab calibration in order to ensure the best detector map for each. This matches well with the 50 revolutions required for the SPAG generation. A re-reading of the collimator measurement report reveals that there is an RMS scatter of lamellae positions (measured at each collimator hole) of 0.1 mm. This implies that the throughput does not have a pyramid shape but rather a rounded apex. /NJW