Imaging dark matter at the smallest scales with z ≈ 1 lensed stars

Open Access

Fig. 10.

Ratio N_near/N_far as a function of β and Σ_* (expressed in units of M_⊙ pc⁻²). The white lines show the combination of β and Σ_* that predict the same number of events in the far and near regions (Ratio = 1) or five time more events in the near region than in the far region (Ratio = 5).

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