Automatic Bayesian inference for LISA data analysis strategies
arXiv:gr-qc/0609010 · doi:10.1063/1.2405082
Abstract
We demonstrate the use of automatic Bayesian inference for the analysis of LISA data sets. In particular we describe a new automatic Reversible Jump Markov Chain Monte Carlo method to evaluate the posterior probability density functions of the a priori unknown number of parameters that describe the gravitational wave signals present in the data. We apply the algorithm to a simulated LISA data set containing overlapping signals from white dwarf binary systems (DWD) and to a separate data set containing a signal from an extreme mass ratio inspiral (EMRI). We demonstrate that the approach works well in both cases and can be regarded as a viable approach to tackle LISA data analysis challenges.
8 pages, 2 sets of figures, submitted to the proceedings of the 6th LISA symposium
Cited by in corpus (7)
- A Solution to the Galactic Foreground Problem for LISA
- Probing black holes at low redshift using LISA EMRI observations
- A Constrained Metropolis-Hastings Search for EMRIs in the Mock LISA Data Challenge 1B
- Improved time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
- Inference on inspiral signals using LISA MLDC data
- Inference on white dwarf binary systems using the first round Mock LISA Data Challenges data sets
- Markov chain Monte Carlo searches for Galactic binaries in Mock LISA Data Challenge 1B data sets