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Fig. 9.

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EPIC spectra of the X-ray burst seen from eRASSt J040515.6 − 745202 (MOS1, black; MOS2, red; and pn, green). The best-fit model consists of two blackbody emission components in addition to the persistent emission. The best-fit model is plotted as a histogram. The two blackbody burst emission components are indicated as green dotted lines and the two components of the persistent emission as blue dotted lines (for better visibility for the pn spectrum only). The bottom panel shows the residuals.

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