JEM-X MONDAY MEETING #73: 10/10-2005
	
SUMMARY;
	Instrument status: Big hotspot is still visible, and so is its little
		companion (see CAO's email about improved hotspot extraction)
		Crab calibration is tonight
	CBJ, Using neural network for position determination: For rev. 363 Carl
		has made pllots of ra-dev and dec-dev against sigma for
		sources found with his program. HUNN is feeding these results
		into a neural network to try to understand remaining 
		systematics. For strongest sources can get down to 4 arc seconds
		of scatter.
	SB, X-ary transient: Type-I burst from XTE J1739-286, last seen a year
		ago, and now seen again this September.
	Gain Correction: SB has circulated a note about the requirements of a
		gain correction and verification module, which everyone should 
		read.
	AOB: JC reports that people in Orsay have complained that JEM-X data
		can't be analysed with OSA 5.0, so they're using OSA4.2. JC
		thinks this may be due to response matrices not yet updated
		at ISDC. [It turned out to be an installation problem at
		Orsay.]