Fig. 7.
Light curve (top) and probability map for mass and distance of the lens (middle) and blended and/or lensed light (bottom) for the event OGLE3-ULENS-PAR-03. This is the nearest (∼600 pc) possible mass-gap object in our sample, with a mass of 
M⊙. The probability that the lens is a dark remnant is 94.5% based on the integrated histogram from the bottom panel.
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