Last updated after receiving ObsID 01014037002, version 8
Data were analysed using HEASOFT version 6.32
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From 2016 March, the light curve plots support interactive zooming and exploring. See the jsPlot
documentation for details.
7 snapshots of PC data are unreliable because no centroid could be determined. 2 bins are affected and have been hidden [Why does this matter?]. List affected times/bins.
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For this burst, 1 count = 5.50 x 10-11 erg cm-2 (observed flux) (Automatic spectrum).
Note that this is an time-averaged conversion factor: the true value may evolve with time.
Generate postscript plot | Data file.
The light curve below shows the unabsorbed luminosity in the GRB comoving frame 0.3-10 keV band. The assumed redshift is 1.046, the photon index is 1.119341594. The counts-to-unabsorbed flux conversion factor is 5.7 x 10-11 erg cm-2 ct-1. The full conversion from counts to luminosity, including distance and k-correction is 1.9 x 1047 erg ct-1. Details were taken from the -mode automated spectral fit Note that these are time-averaged values: the true properties may evolve with time.
Generate postscript plot | Data file.
Generate postscript plot | Data file.
Generate postscript plot | Data file.
Download all light curve files for this burst: [tar file][gzipped tar file][zip file].
Or download individual files: (Includes systematic error. Includes data with no WT centroid.)