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Fig. 1.

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Best-fit parameters of the burst recorded in ObsID 2050300110. From top to bottom: 0.1–20 keV bolometric X-ray luminosity in units of 1038 erg s−1 assuming a 8 kpc distance, the 0.3–10 keV count rate (counts/s), the inferred blackbody radius (km), the blackbody temperature (keV), and the fa parameter. The green area defines the time period during which the inferred blackbody radius was larger than 100 km. All errors are given at the 90% confidence level.

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