Swift-XRT light curve of GRB 050520 - INTEGRAL burst

Last updated using ObsID 04022572008, version 18

Details of how these lightcurves were made are given in Evans et al. (2007). Please cite this paper if you use these data. Also, please include the following sentence in the acknowledgements of any publication which uses these data: This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester.

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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.

The images below link to the ASCII data

Basic Lightcurve

Detailed Lightcurve

$Lightcurve of GRB 050520 - INTEGRAL burst, including background level and fractional exposure$

Summed PC-mode image - exposure time: 15.21 ks

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