Low-rank approximations for large stationary covariance matrices, as used in the Bayesian and generalized-least-squares analysis of pulsar-timing data
arXiv:1407.6710 · doi:10.1093/mnras/stu2157
Abstract
Many data-analysis problems involve large dense matrices that describe the covariance of stationary noise processes; the computational cost of inverting these matrices, or equivalently of solving linear systems that contain them, is often a practical limit for the analysis. We describe two general, practical, and accurate methods to approximate stationary covariance matrices as low-rank matrix products featuring carefully chosen spectral components. These methods can be used to greatly accelerate data-analysis methods in many contexts, such as the Bayesian and generalized-least-squares analysis of pulsar-timing residuals.
arXiv comment6 pages, 3 figures
References in corpus (8)
- Assessing the Role of Spin Noise in the Precision Timing of Millisecond Pulsars
- On measuring the gravitational-wave background using Pulsar Timing Arrays
- TempoNest: A Bayesian approach to pulsar timing analysis
- Pulsar timing analysis in the presence of correlated noise
- Understanding and analysing time-correlated stochastic signals in pulsar timing
- NANOGrav Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries in Circular Orbits
- Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data
- New advances in the Gaussian-process approach to pulsar-timing data analysis
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