Fig. A.1.
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Comparison of DRS-extracted and custom-extracted correlated fluxes for Circinus (left) and a calibration star, HD120404 (right). From top to bottom, the panels show the cleaned fringe pattern (the Fourier transform of the cleaned interferogram), the six fringes extracted with the DRS, and the same six fringes extracted with our method. In the Circinus fringe pattern, there is significant flux in the M band that is missing in the DRS fringes but is present in our method.
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