Estimation of Parameters of Gravitational Waves from Pulsars
Andrzej Kr\'olak (Max Planck Institute for Gravitational Physics, The, Albert Einstein Institute, Potsdam, Germany On leave of absence from, Institute of Mathematics, Polish Academy of Sciences, Warsaw, Poland)
TL;DR
This paper discusses methods for estimating parameters of nearly periodic gravitational wave signals from pulsars using laser interferometric data, focusing on accuracy and computational efficiency.
Contribution
It introduces a simple model for gravitational wave signals from pulsars and evaluates parameter estimation accuracy and computational demands.
Findings
Parameter estimation accuracy assessed
Computational requirements analyzed
Model simplifies gravitational wave signal analysis
Abstract
The problem of search for nearly periodic gravitational wave sources in the data from laser interferometric detectors is discussed using a simple model of the signal. Accuracies of estimation of the parameters and computational requirements to do the search are assessed.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements