On 25Apr18: 6 Events were detected

• 📁 **25Apr18**
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•     📁 **pi1-events-25Apr18**
•        📄 25-04-18T170807_372
•        📄 25-04-18T215824_798
•     📁 **pi10-events-25Apr18**
•        📄 25-04-18T023508_238
•        📄 25-04-18T170807_315
•     📁 **pi11-events-25Apr18**
•        📄 25-04-18T155049_899
•        📄 25-04-18T170807_230
•     📁 **pi3-events-25Apr18**
•        📄 25-04-18T023508_475
•        📄 25-04-18T155049_900
•        📄 25-04-18T170807_145
•        📄 25-04-18T175530_755
•        📄 25-04-18T215824_760
•        📄 25-04-18T224208_963
•     📁 **pi5-events-25Apr18**
•        📄 25-04-18T023508_488
•        📄 25-04-18T170807_374
•        📄 25-04-18T175530_751
•        📄 25-04-18T215824_719
•        📄 25-04-18T224208_958
•     📁 **pi6-events-25Apr18**
•        📄 25-04-18T155049_894
•        📄 25-04-18T170807_349
•        📄 25-04-18T175530_879
•        📄 25-04-18T224209_092

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 25Apr18  17.082+/-0.086  0.201 170455.676       60783.7118   131.0+/- 7.3 

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