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Swift-XRT light curves of GRB 080330

Last updated after receiving ObsID 00308041009, version 14

Data were analysed using HEASOFT version 6.29

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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 WT data are unreliable because no centroid could be determined. 10 bins are affected and have been hidden [Why does this matter?]. List affected times/bins.

57 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.

Flux Conversion

   [What is this?][View systematics and position variation]

To convert from counts to flux requires knowledge of the GRB spectrum. This is not automatically generated. The mean conversion factor from count rate to observed flux (0.3-10 keV) for 10 GRBs between GRB 070110 and GRB070306 is 1 count s-1 = 5x10-11 erg cm-2s-1, with a standard deviation of 2.6x10-11 erg cm-2s-1. The GCN report for this GRB will give a more accurate value, specifically calculated for this burst. When this is available, a flux light curve will appear here.

Basic Light Curve

   [What is this?][View systematics and position variation]

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Detailed Light Curve

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Hardness Ratio

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DETX and systematic error

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Generate postscript plot | Data file.

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Data products

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.)