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Fig. 8.


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EPIC spectra of the persistent emission from eRASSt J040515.6 − 745202 (MOS1, black; MOS2, red; and pn, green) extracted from the full observation, excluding the burst interval. The best-fit model consisting of a disk-blackbody and a power-law component is plotted as histogram. The two emission components are indicated as dotted lines (for better visibility for the pn spectrum only). The bottom panel shows the residuals.

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