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  • Masa and James have finished coding the blind search tool gtspec. Testing on DC2 data is underway.

Observation simulation

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  • From Max Razzano:
    • "EGRET phase-dependent sources, fixes and extended down to 10 MeV. The lightcurve have been smoothed for the 3 faintest (no phase-dependence) and for Vela, Crab and Geminga we have phase dependent spetcrum and also some very narrow features that we can use for testing timing resolution;
    • "Timing noise on 5 pulsars, based on Cordes algorithm of Random Walk(in phase) and of Arzoumanian (f2 based on Delta8 parameter);
    • "3 MSP in binary orbits, we have this last problem but I solved and it is ok;"

User interface and infrastructure (& utilities)

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