Fig. 2
Top: TPF of WASP-33 showing the chosen aperture mask. No stars can be visually resolved. Bottom: field of view of about 4 × 4 arcmin centered on WASP-33. The mask and pixels are schematized with white thick and thin lines, respectively. WASP-33C, the bright star south of WASP-33, is not included in the aperture. The field of view has been rotated to be aligned with the ecliptic system, and is oriented to coincide with the images given in the TESS summary report.
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