Fig. 10.

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DarkLensCode output for the GO+ microlensing model assuming the StellarIMF mass function. Posterior distribution of the blended light magnitude and lens light magnitude assuming that the lens is an MS star. The solid line represents the upper limit of extinction, while the dashed line represents the lower limit of extinction. Lines separate the dark lens solutions from the MS star solutions. The colours correspond to the log probability density. Black bins are those containing no samples.
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