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GRB 050215A
The Swift Burst Analyser — GRB 050215A
Last updated using ObsID 00106106000, version 16;
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=0.149 × 1022 cm-2 at z=0 and 1.00 × 1022 cm-2 at z=2.23.
(Source: typical values from Evans et al. 2009).
Observed BAT flux
■ BAT
Observed flux density, with photon index sub plot. BAT binning: SNR 5.
Show full observed flux Observed flux density plot controls.
Generate postscript plot | Data file.
BAT unabsorbed flux light curves
Flux density at 10 keV, with photon index sub plot. BAT binning: SNR 5.
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 96, from -23.9 to 72.0
The spectral fit used was a power-law with photon index: 1.32
Count-rate light curves are available from GCN.
BAT unabsorbed flux light curves, no spectral evolution
Flux density at 10 keV. BAT binning: SNR 5.
Show full BAT, no spectral evolution Flux density at 10 keV plot controls.
Generate postscript plot | Data file.