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Analysis of the noise background of the “ULITKA” gravitational antenna

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Abstract

A long-term analysis of the noise background of the “ULITKA” gravitational-wave antenna is presented in connection with searches for anomalous impulsive signals and slow solar-terrestrial correlations with a period of 27 days. Automated selection and estimation algorithms are used, including nonparametric criteria for the statistical dependence of samples uniform in time. The upper limit for the gravitational-noise background is confirmed by the observational statistics. The presence of slow, anomalous correlations is not confirmed.

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992, Russia

    A. V. Gusev, V. N. Rudenko & A. V. Serdobol'skii

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  1. A. V. Gusev
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  2. V. N. Rudenko
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  3. A. V. Serdobol'skii
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__________

Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 80, No. 8, 2003, pp. 728–737.

Original Russian Text Copyright © 2003 by Gusev, Rudenko, Serdobol'ski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \).

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Gusev, A.V., Rudenko, V.N. & Serdobol'skii, A.V. Analysis of the noise background of the “ULITKA” gravitational antenna. Astron. Rep. 47, 670–678 (2003). https://doi.org/10.1134/1.1601635

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  • DOI: https://doi.org/10.1134/1.1601635

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