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...in this paper a Bayesian parameter estimation method for the
analysis of interferometric gravitational wave observations of an inspiral of
binary compact objects using data recorded simultaneously by a network of
several interferometers at different sites. We consider neutron star or black
hole inspirals that are modeled to 3.5 post-Newtonian (PN) order in phase and
2.5 PN in amplitude. Inference ...
http://vsevcosmos.livejournal.com/26026698.html
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Published: 1 year, 11 months ago (Sat, 28 Jul 2007 06:02:12 PDT); 1581 bytes
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