Using weighting algorithms to refine source direction determinations in all-sky gravitational wave burst searches with two-detector networks II: The case of elliptical polarization
arXiv:2003.13455
Abstract
I expand on the results of a recent work in which a novel weighting algorithm was shown to substantially increase the accuracy of an old, non-Bayesian computational approach for inferring the source direction of a gravitational wave from the output of a two-detector network. While that work was limited to the consideration of circularly polarized gravitational waves, the current analysis shows that the same approach is even more successful when applied to the generic case of elliptically polarized gravitational waves.
arXiv comment27 pages, 17 figures. arXiv admin note: text overlap with arXiv:1805.01309
References in corpus (5)
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
- Localization of gravitational wave sources with networks of advanced detectors
- All-sky search for short gravitational-wave bursts in the first Advanced LIGO run
- Localization of short duration gravitational-wave transients with the early advanced LIGO and Virgo detectors
- Parameter estimation for gravitational-wave bursts with the BayesWave pipeline