Fig. 5.
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Marginalised posterior probability density functions for the fraction of DM in PBHs, fPBH, for the galaxies Triangulum II (upper panels) and Segue 1 (lower panels), adopting the BPL (left panels) and LN (right panels) IMFs. One-sided 1σ, 2σ, and 3σ intervals are displayed with colours ranging from darker to lighter shades. The grey region corresponds to fPBH > 1.
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