On 25Apr05: 7 Events were detected

• 📁 **25Apr05**
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•     📁 **pi1-events-25Apr05**
•        📄 25-04-05T224936_035
•        📄 25-04-05T225512_290
•        📄 25-04-05T230442_236
•        📄 25-04-05T231107_954
•        📄 25-04-05T232017_610
•     📁 **pi10-events-25Apr05**
•        📄 25-04-05T180157_814
•        📄 25-04-05T210417_014
•     📁 **pi3-events-25Apr05**
•        📄 25-04-05T180157_625
•        📄 25-04-05T210416_980
•        📄 25-04-05T224936_038
•        📄 25-04-05T225512_285
•        📄 25-04-05T230442_262
•        📄 25-04-05T231107_945
•        📄 25-04-05T232017_617
•     📁 **pi5-events-25Apr05**
•        📄 25-04-05T180157_630
•        📄 25-04-05T210416_990
•        📄 25-04-05T224936_049
•        📄 25-04-05T225512_290
•        📄 25-04-05T230442_235
•        📄 25-04-05T231107_952
•        📄 25-04-05T232017_600
•     📁 **pi6-events-25Apr05**
•        📄 25-04-05T224936_022
•        📄 25-04-05T225512_283
•        📄 25-04-05T230442_235
•        📄 25-04-05T231107_943
•        📄 25-04-05T232017_616

Successfully fit 1 Event Group.
When many flashes are detected we fit the average time of events
FWHM is the time interval of gaussain fit, in hours
#     Date        Fit Hour    FWYM  HHmmSS.sss         MJD        Event Counts
#FIT 25Apr05  23.363+/-0.060  0.142 232147.580       60770.9735   671.0+/-20.0 

Overview of Radio Detection of Cosmic Ray Flashes and access to observations.