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Fig. 1.


PSF-matching for the binary 2M2202. Upper left and right plots: observed data and PSF of the standard star used, respectively. Lower left plot: best fit of a constructed model made from two reference PSFs that we match to the positions and scale with the brightness of the two components. Lower right plot: residuals after subtracting the model from the observed data. All plots have been normalized to match the observed data.

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