Fermi-GBM SFL100810049 Summary
Trigger Summary
Trigger Time [MET] : 303095436.242630
Burst Pos RA [deg] : 117.8333
Burst Pos Dec [deg] : -9.1667
Burst Err Radius [deg] : 34.3167
Trigger significance [sig]: 4.8
Trigger time scale [ms] : 1024
Trigger channel low : 3
Trigger channel high : 4
Trigger channel low (ADC) : 259
Trigger channel high (ADC): 1352
Triggered detector : 00010100000000
SC Geo East Long [deg] : 120.2274
SC Geo North Lat [deg] : 21.2185
GBM Light curves
Notes:
- 1) The data are from the Fermi-SDC: http://heasarc.gsfc.nasa.gov/FTP/fermi/data/
- 2) The light curve is generated using the Fermi-tool gtbin for the TTE data.
- 3) The individual panel shows the GBM light curve for each GBM detector (GBM-BGO: b0 and b1, GBM-NaI: from n0 to nb) in full energy range.
1s binning
All interval
From T0-10 to T0+100
From T0-10 to T0+50
From T0-10 to T0+10
64ms binning
All interval
From T0-10 to T0+100
From T0-10 to T0+50
From T0-10 to T0+10
LAT Sky Image
Notes:
- 1) The data are from the LAT photon server: http://fermi.gsfc.nasa.gov/FTP/fermi/data/lat/allsky/
- 2) The LAT image is created using the Fermi-tool gtselect and gtbin.
- 3) The GBM position with 35 degree radius is used to create the image.
- 4) The energy ranges are from 100 MeV to 300 GeV and from 1 MeV and 100 MeV (basically less than 100 MeV).
- 5) The image is searched using ximage detect command. If ximage detect command finds any significant source, the result is shown at the bottom of the image
- 6) Green circle is the GBM error circle.
- 7) Time stamp of the last LAT event in the process is 303099761.430814
100 MeV - 300 GeV
less than 100 MeV
LAT light curves
Notes:
- 1) All the photons within a radius of 35 degrees from the GBM position are used to construct the light curve (because the GBM location is not that accurate).
1s binning
10s binning
GBM-LAT light curve (1s binning)
Notes:
- 1) GBM light curves are from the triggered detectors.
GBM + 100 MeV-300 GeV LAT light curves
GBM + 1 MeV-100 MeV LAT light curves
