Fig. 1
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Variation in the stellar colors V -I (red) and B-R (green) versus the magnification factor due to the BL effect. The adopted blending parameters, given in the figure, are the average of blending parameters for simulated microlensing events toward the Baade’s window, with the coordinate (lG = 1°, bG = − 4°), by excludinghighly blended events with bI < 0.2.
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