Last updated after receiving ObsID 00599287001, version 5
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.
1 snapshots of PC data are unreliable because no centroid could be determined. 1 bins are affected and have been hidden [Why does this matter?]. List affected times/bins.
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For this burst, 1 count = 3.40 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.
[What is this?][View systematics and position variation]
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 4.707, the photon index is 1.909993166. The counts-to-unabsorbed flux conversion factor is 3.8 x 10-11 erg cm-2 ct-1. The full conversion from counts to luminosity, including distance and k-correction is 7.8 x 1048 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.
[What is this?][View systematics and position variation]
Generate postscript plot | Data file.
[What is this?][View systematics and position variation]
Generate postscript plot | Data file.
[What is this?][View systematics and position variation]
Generate postscript plot | Data file.
[What is this?][View systematics and position variation]
Generate postscript plot | Data file.
View systematics and position variation
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.)