Poster + Paper
23 August 2024 Tunable kernel-nulling interferometry for direct exoplanet detection
Vincent Foriel, Frantz Martinache, David Mary
Author Affiliations +
Conference Poster
Abstract
Nulling interferometry is a promising technique for direct detection of exoplanets. However, the performance of current devices is limited by the sensitivity to phase aberrations. The work presented here attempts to overcome those challenges by using a four-telescopes nulling interferometer architecture, called Kernel-Nuller, which includes a recombiner that positions the four signals in phase quadrature. This architecture is based on an integrated optical component containing 14 electronically controlled phase shifters, used to correct optical path differences that would be induced by manufacturing defects. The first part of the study consists in the development of an algorithm providing the delays to be injected into the component to optimize the performance of that device. The next step of this study deals with the analysis of the intensity distributions produced at the output of the Kernel-Nuller through a series of observations, against which statistical tests and data treatment techniques are applied to detect the presence of exoplanets.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Vincent Foriel, Frantz Martinache, and David Mary "Tunable kernel-nulling interferometry for direct exoplanet detection", Proc. SPIE 13092, Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave, 130925X (23 August 2024); https://doi.org/10.1117/12.3019726
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KEYWORDS
Phase shifts

Exoplanets

Nulling interferometry

Planets

Telescopes

Calibration

Modulation

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