Estimation of the signal parameters in a gravitational-wave detection experiment

Details Estimation of the signal parameters in a gravitational-wave detection experiment Estimation of the signal parameters in a gravitational-wave detection experiment

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..367t&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 367-376. In Russian.

Astronomy and Astrophysics

Astronomy

Algorithms, Gravitational Effects, Gravitational Wave Antennas, Signal Distortion, Least Squares Method, Maximum Likelihood Estimates, Parameter Identification, Signal To Noise Ratios

Scientific paper

It is shown that the maximum likelihood (ML) algorithm for estimating the parameters of a gravitational-radiation burst does not require additional a priori information for its implementation. The application of this algorithm does not lead to a significant increase in the volume of computer calculations in comparsion with the least squares method. It is shown that, in general, the application of the ML method makes it possible to improve the accuracy of the estimation of gravitational-radiation burst parameters, which has important implications for gravitational-wave detection experiments.

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