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We are studying the feasibility of using a rotational shearing interferometer to detect a planet in a nearby solar system. In this paper, we describe the status of our work. We built a rotationally shearing interferometer and demonstrated that a simulated star indeed produces a field without fringes. The faint simulated planet provokes appearance of faint fringes. Their density and slope may be changed upon changing the shear angle when the planet is present.
Marija Strojnik
"Rotationally shearing interferometry in the recovery of faint signals", Proc. SPIE 11830, Infrared Remote Sensing and Instrumentation XXIX, 1183007 (1 August 2021); https://doi.org/10.1117/12.2598438
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Marija Strojnik, "Rotationally shearing interferometry in the recovery of faint signals," Proc. SPIE 11830, Infrared Remote Sensing and Instrumentation XXIX, 1183007 (1 August 2021); https://doi.org/10.1117/12.2598438