Fig. 3
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Comparison between the cumulative XLF of the LMC. The XLF obtained in Maggi et al. (2016) is shown in black, while the eROSITA XLF for which the luminosities were determined as described in Sect. 5.1 is shown in red, and the eROSITA luminosities obtained using the ECF assuming an apec model with kT = 0.5 keV and NH = 0.25 × 1022 cm−2 are in blue.
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