Detection of signals at the output of gravity resonance antennas by estimation of the distribution parameters
Author:
Publisher
Springer Science and Business Media LLC
Subject
Applied Mathematics,Instrumentation
Link
http://link.springer.com/content/pdf/10.1007/s11018-011-9716-x.pdf
Reference7 articles.
1. P. Astone et al., “Search for time correlation between gramma-ray bursts and data from the gravitational wave antenna EXPLORER,” Astron. and Astrophys., Suppl., 138, No. 3 (1999).
2. P. Astone et al., “Search for coincident excitation of the widely spaced resonant gravitational wave detectors EXPLORER, NAUTILUS, and NIOBE,” Astropart Phys., 10, No. 1 (1999).
3. A. S. Akimov et al., Signal Detection Theory [in Russian], Radio i Svyaz, Moscow (1984).
4. V. N. Rudenko and A. V. Gusev, “Nonlinear algorithm of searching for astro-gravity correlations,” Intern. J. Modern Physics. D, 9, No. 3, 353–359 (2000).
5. A.V. Gusev and V. N. Rudenko, “Optimal recognition of gravitational signals,” Izmer. Tekhn., No. 5, 8–11 (2010); Measur. Techn., 53, No. 5, 471–475 (2010).
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