GRB 090107
Last updated using ObsID 00339295000, version 6;
Data were analysed using HEASOFT version 6.11
From 2016 January, the light curve plots support interactive zooming and exploring. See the jsPlot
documentation for details.
Also, from the same date, the first plot on this page is the observed flux
in the native band of each instrument (including UVOT where available).
Jump to: Observed flux | BAT | BAT no evolution.
Downloads: BAT spectral evolution data | All files for this object: [tar][tar.gz][zip].
All data uses absorption NH=0.100 × 1022 cm-2 at z=0 and 1.00 × 1022 cm-2 at z=2.23.
(Source: typical values from Evans et al. 2009).
■ BAT
Show full observed flux Observed flux density plot controls.
Generate postscript plot | Data file.
Show full BAT Flux density at 10 keV plot controls.
Generate postscript plot | Data file.
The fit to the T90 spectrum was used to create the plots in this section.
T90 was 12.3, from 0.3 to 12.6
The spectral fit used was a power-law with photon index: 1.81
Count-rate light curves are available from GCN.
Show full BAT, no spectral evolution Flux density at 10 keV plot controls.
Generate postscript plot | Data file.