Fig. 24

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Magnification probability for a case with ∑eff/∑crit = 2, in both parity regimes. This mimics the magnification probability of a hypothetical microlensing population consisting of 5 M⊙/pc2 stars and 20 M⊙ pc−2 PBHs. The critical density is ∑crit = 2500 M⊙ pc−2. μt = 200 and μr = 4. Left panel: negative macro-magnification. Right panel: positive macro-magnification. The dashed curve represents the magnification probability for the same system with no PBHs.
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