LISA Data Analysis using MCMC methods
Neil J. Cornish, Jeff Crowder

TL;DR
This paper demonstrates the successful application of MCMC methods to analyze simulated LISA gravitational wave data, effectively identifying signals and estimating parameters in a complex, high-dimensional space.
Contribution
It introduces the first use of MCMC techniques for LISA data analysis, showcasing their efficiency in handling large parameter spaces and overlapping signals.
Findings
MCMC accurately identifies the number of signals.
Parameter estimates are consistent with Fisher matrix predictions.
The approach effectively explores a 50,000-dimensional parameter space.
Abstract
The Laser Interferometer Space Antenna (LISA) is expected to simultaneously detect many thousands of low frequency gravitational wave signals. This presents a data analysis challenge that is very different to the one encountered in ground based gravitational wave astronomy. LISA data analysis requires the identification of individual signals from a data stream containing an unknown number of overlapping signals. Because of the signal overlaps, a global fit to all the signals has to be performed in order to avoid biasing the solution. However, performing such a global fit requires the exploration of an enormous parameter space with a dimension upwards of 50,000. Markov Chain Monte Carlo (MCMC) methods offer a very promising solution to the LISA data analysis problem. MCMC algorithms are able to efficiently explore large parameter spaces, simultaneously providing parameter estimates,…
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