Fig. 20.

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Total expected LX/SFR distribution due to stochastic sampling of HMXBs XLF as a function of the sSFR. The rhombuses indicate the mean LX/SFR per SFR-M⋆ bin, colour-coded with the gas phase metallicity. The orange and magenta lines correspond to the upper and lower 99%, and 99.9% C.Is. of the HMXBs expected LX/SFR, respectively. Grey dashed line depicts the upper 99.9% C.I of the total expected luminosity accounting for the stochasticity of both, LMXBs and HMXBs. We also overplot with a red line the LX/SFR – sSFR L16 scaling relation, and its corresponding 1σ scatter.
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