On 25Aug23: 6 Events were detected

• 📁 **25Aug23**
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•     📁 **pi11-events-25Aug23**
•        📄 25-08-23T121402_464
•        📄 25-08-23T165655_058
•        📄 25-08-23T170546_224
•        📄 25-08-23T205643_583
•     📁 **pi3-events-25Aug23**
•        📄 25-08-23T002612_373
•        📄 25-08-23T023857_215
•        📄 25-08-23T121402_550
•        📄 25-08-23T165655_091
•        📄 25-08-23T170546_234
•        📄 25-08-23T205643_810
•     📁 **pi5-events-25Aug23**
•        📄 25-08-23T165655_051
•        📄 25-08-23T205643_733
•     📁 **pi6-events-25Aug23**
•        📄 25-08-23T002612_465
•        📄 25-08-23T023857_114
•        📄 25-08-23T165655_238
•        📄 25-08-23T170546_225
•        📄 25-08-23T205643_713
•     📁 **pi9-events-25Aug23**
•        📄 25-08-23T002612_363
•        📄 25-08-23T023857_208
•        📄 25-08-23T121402_452
•        📄 25-08-23T165655_112
•        📄 25-08-23T170546_175
•        📄 25-08-23T205643_701

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 25Aug23  16.953+/-0.082  0.193 165709.182       60910.7064   293.0+/-11.4 

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