On 25Jun23: 5 Events were detected

• 📁 **25Jun23**
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•     📁 **pi10-events-25Jun23**
•        📄 25-06-23T203059_030
•        📄 25-06-23T205205_072
•        📄 25-06-23T234938_264
•        📄 25-06-23T235527_087
•     📁 **pi11-events-25Jun23**
•        📄 25-06-23T203058_584
•        📄 25-06-23T234938_053
•        📄 25-06-23T235527_042
•     📁 **pi5-events-25Jun23**
•        📄 25-06-23T150019_851
•        📄 25-06-23T203058_830
•        📄 25-06-23T205205_180
•        📄 25-06-23T234938_185
•        📄 25-06-23T235527_037
•     📁 **pi6-events-25Jun23**
•        📄 25-06-23T150019_778
•        📄 25-06-23T203058_833
•        📄 25-06-23T205205_378
•        📄 25-06-23T235527_041
•     📁 **pi9-events-25Jun23**
•        📄 25-06-23T150019_777
•        📄 25-06-23T203058_823
•        📄 25-06-23T205205_223
•        📄 25-06-23T234938_253
•        📄 25-06-23T235527_032

Successfully fit 2 Event Groups.
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 25Jun24  24.333+/-0.118  0.278 002000.016       60850.0139  9454.0+/-861.6 

#FIT 25Jun23   0.227+/-0.161  0.380 001338.980       60849.0095  7822.4+/-98.3 

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