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Fig. 11

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(1 − f)   c1exp(−c2|b|)  ×  10-6 fit to the OGLE, MACHO, and EROS bright stars optical depth data (solid line) and a similar fit to the narrowed data of MACHO and EROS bright stars data (dashed line). The filled area corresponds to the standard deviation range of the Monte Carlo simulation (including bar) described in the previous section. The c1exp(−c2|b|)  ×  10-6 curve is not plotted for clarity.

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