Fig. 2.
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Differential form of the synthetic XLFs, showing the default population (solid blue line) compared to the observed XLF from Lehmer et al. (2019, pink shaded region). The population is further split by the type of XRB (RLO or wind), type of accretor (BH or NS), and type of donor (H-rich or He-rich). Be XRBs are shown with a dotted gray line.
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