Fig. 10
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HR versus flux for eRASS1 Galactic plane sources. Upper panel: HR against the 0.2-8 keV flux for eRASS1 sources within |b| < 1°. The vertical dashed line represents an empirical cut at HR=-0.2. Known Galactic LMXBs and HMXBs from Avakyan et al. (2023) and Neumann et al. (2023) are indicated by blue and orange squares, respectively. Lower panel: HR histograms for different source categories.
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