Nulling interferometer differential-output noise is non-Gaussian and approximately follows an iteratively convolved Bessel distribution, so Gaussian significance thresholds are overconfident and need a correction factor.
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Consequences of Non-Gaussian Instrumental Noise in Perturbed Nulling Interferometers
Nulling interferometer differential-output noise is non-Gaussian and approximately follows an iteratively convolved Bessel distribution, so Gaussian significance thresholds are overconfident and need a correction factor.