Difference between revisions of "Parameter estimation of compact binaries"
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| − | The estimation of parameter values and associated waveforms of observed compact-binary coalescences is an important contribution to the science case of GW detectors. It is key to tests of general relativity, to many cosmological studies, to population studies of compact objects, to studies of gravitational lensing of gravitational waves, of course, to the exploration of the nature and properties of the objects involved in the merger | + | The estimation of parameter values and associated waveforms of observed compact-binary coalescences is an important contribution to the science case of GW detectors. It is key to tests of general relativity, to many cosmological studies, to population studies of compact objects, to studies of gravitational lensing of gravitational waves, and of course, to the exploration of the nature and properties of the objects involved in the merger. |
[[http://dx.doi.org/10.3847/1538-4365/ab06fc Ashton et al (2019)]] | [[http://dx.doi.org/10.3847/1538-4365/ab06fc Ashton et al (2019)]] | ||
Revision as of 14:40, 15 September 2020
The estimation of parameter values and associated waveforms of observed compact-binary coalescences is an important contribution to the science case of GW detectors. It is key to tests of general relativity, to many cosmological studies, to population studies of compact objects, to studies of gravitational lensing of gravitational waves, and of course, to the exploration of the nature and properties of the objects involved in the merger.
