10:45 AM–12:21 PM, Saturday, April 12, 2008
Hyatt Regency St. Louis Riverfront (formerly Adam's Mark Hotel), - St. Louis A
Sponsoring Units:
GGR DAP
Chair: Duncan Brown, Syracuse University
Abstract ID: BAPS.2008.APR.B10.4
11:21 AM–11:33 AM
Marc van der Sluys
Christian Roever
Alexander Stroeer
Nelson Christensen
Vicky Kaloger
Renate Meyer
Alberto Vecchio
Ilya Mandel
We present a Markov-Chain Monte-Carlo (MCMC) technique to study the source parameters of signals from the inspirals of stellar-mass compact binaries observable with ground-based gravitational-wave detectors such as LIGO and Virgo. We use a number of modifications to the standard MCMC in order to efficiently probe the parameter space while keeping the algorithm suitable for a wide range of signals. We shall discuss the performance of the MCMC algorithm and the typical measurement accuracy of the source parameters as a function of the binary parameters and the number of detectors in the network. We will show that despite the lower positional accuracy compared to other astronomical observations, an association of a gravitational- wave event with e.g. an electomagnetic detection is possible with three or even two 4-km-size interferometers.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2008.APR.B10.4