Modelling coloured residual noise in gravitational-wave signal processing

Details Modelling coloured residual noise in gravitational-wave signal processing Modelling coloured residual noise in gravitational-wave signal processing

2008-04-24

arxiv.org/abs/0804.3853v6

Classical and Quantum Gravity 28:015010, 2011

Statistics

Methodology

21 pages, 5 figures

Scientific paper

10.1088/0264-9381/28/1/015010

We introduce a signal processing model for signals in non-white noise, where the exact noise spectrum is a priori unknown. The model is based on a Student's t distribution and constitutes a natural generalization of the widely used normal (Gaussian) model. This way, it allows for uncertainty in the noise spectrum, or more generally is also able to accommodate outliers (heavy-tailed noise) in the data. Examples are given pertaining to data from gravitational wave detectors.

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