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Fig. 1.

image

BAT and XRT light curves of all 28 X-ray bursts with BAT event files and followed up with XRT, except 4U 1812-12/2005-02-24 because its XRT coverage is sparse. The BAT light curves are normalized and corrected for a changing pointing due to the slews. The XRT data are for the complete detector and without corrections for pile-up or background. The steps that can sometimes be seen in XRT data are due to a switch in CCD data collection mode with different pile-up fractions.

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