Fig. 6.
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Constraints on 1019g asteroid-mass PBHs from this work. The dot corresponds to the maximum of the posterior distribution of fPBH, whose value is consistent with fPBH = 0. To the left and the right, we show the existing constraints on PBHs arising from evaporation and microlensing, plotted using the data compiled in the PBH bounds repository (https://github.com/bradkav/PBHbounds).
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