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Parametric Estimation of the Threshold when Detecting Weak Gravitational Pulses

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Measurement Techniques Aims and scope

Abstract

It is proposed to utilize the integral distribution function of the absolute maximum of a bi-Gaussian random process in order to calculate the threshold when detecting weak gravitational pulses on a non-Gaussian noise background.

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Authors
  1. A. V. Gusev
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  2. A. Yu. Kochetkova
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Gusev, A.V., Kochetkova, A.Y. Parametric Estimation of the Threshold when Detecting Weak Gravitational Pulses. Measurement Techniques 44, 903–907 (2001). https://doi.org/10.1023/A:1013299403561

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  • DOI: https://doi.org/10.1023/A:1013299403561

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