List of transients observed by the GRB detector on the GRBBeta nanosatelite

• Event type/name denotes the type of the detected event like GRB, Solar flare etc.
• Ch. no. is the readout channel number of the detector (0 or 1)
• Peak time denotes the time when the detected count rate from the event was maximal
• T90 is the time interval, in which 90 per cent of all counts in the given energy band from the event are observed
• Peak count rate is the detected count rate of the event at the peak time
• Band is the energy range for which the T90 duration and the count rate was calculated
• S/N is the maximal significance of the signal detected in any of the energy bands (either in one bin at the peak or integrated over T90)
• Raw LC is the raw light curve without the background subtraction
• Bkg-sub LC is the light curve with background subtracted
• LC res. is the light curve resolution
• GCN circ. is the GCN circular number where this detection was reported
• References give the list of other instruments which detected the same event

Contacts:

Return to High Energy Astrophysics Group