Subject: JEMX Monday Meeting 2004-10-18



Present: CAO, NL, JC, ILR, NJW

JEMX status: The dead anode observed by Peter Kretschmar was already seen
           by JC.
           
           JC: The Xe peak continues to move up in energy with time, now perhaps
           even faster (in JMX1). Should one of the FRSS sources be excluded
           from the fit in j_cor_gain ? CAO will make some investigations.
           
           ILR: The patch for getting peak countrates of short/strong bursts
           with high time resolution is about to be ready. An extra event
           with hardware triggernumber inserted in place for cathode position,
           delta-time of zero and very high energy (to exclude it from
           processing in analysis) will be issued when a 5-buffer loss
           has occurred a certain number of times.
           
Science analysis workshop: NL, SB, and NJW went there and found that it had
           been fruitful. Good idea to get hands on ISGRI analysis in particular
           with the experts around.
           
OSA4.2     CAO has delivered her components.
           NJW has shadowgram/basic_reconstruction ready but not delivered
OSA5       NL tells that the coming j_ima_iros uses most of its time by
           reading in the ~400 MB data when dealing with a single shadowgram.
           Can the pipeline be ordered by level rather than by science window?
           This is a question for ISDC (Peter Kretschmar and Silvia Martinez).
           
AO3 proposals:  Due very soon.

/NJW

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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