Fig. 3
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Contrast ratio of TOI-1736 as a function of angular separation at 562 nm (blue line) and at 832 nm (red line) obtained from the ‘Alopeke/Gemini speckle imaging observations. The small panels show the reconstructed speckle image (right subpanel) and its power spectrum in Fourier space (left subpanel). The power spectrum shows fringes that match a binary model.
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