Abstract
A common technique for detection of gravitational-wave signals is searching for excess power in frequency-time maps of gravitational-wave detector data. In the event of a detection, model selection and parameter estimation will be performed in order to explore the properties of the source. In this paper, we develop a Bayesian statistical method for extracting model-dependent parameters from observed gravitational-wave signals in frequency-time maps. We demonstrate the method by recovering the parameters of model gravitational-wave signals added to simulated advanced LIGO noise. We also characterize the performance of the method and discuss prospects for future work.
Original language | English |
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Article number | 165012 |
Journal | Classical and quantum gravity |
Volume | 31 |
Issue number | 16 |
DOIs | |
Publication status | Published - 5 Aug 2014 |
Keywords / Materials (for Non-textual outputs)
- gr-qc