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Fig. C.1

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Distribution of average line-of-sight velocities for a simulated population of stars with 50% binary fraction, observed with the same cadence as our sample of Hot Stars, and with the same vl.o.s. errors. Vertical lines mark the 16th/84th percentile for single (dashed) and binary (dotted) stars. Annotated labels report the mean and corresponding uncertainty intervals derived from the 16th and 84th percentiles.

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