SLIDE 8 Background Projects Results Collaboration Support Performance Evaluation Operations Support
InterPlanetary Network
Software Features
Generate high-res lightcurve from TTE data Choose detectors to maximize signal-to-noise Correctly adjust for leap seconds and deadtime Format output for use by existing software
Count Rate [cps]
Comparison of GRB Lightcurves
IPN 1000 1500 2000 2500 3000 Count Rate [cps] CTIME 1000 1500 2000 2500 3000 Count Rate [cps] Time from Trigger [s] CSPEC 1000 1500 2000 2500 3000
2 4 6 8 10 12
The InterPlanetary Network uses observations from multiple spacecraft to pinpoint a burst’s location.
Curran D. Muhlberger, Charles A. Meegan On-Orbit Performance of the GLAST Burst Monitor