Difference between revisions of "Parameter estimation of compact binaries"
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[[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)]] | ||
| − | [[Cosmology:_Probing_the_Early_Universe Cosmology]] | + | [[Cosmology:_Probing_the_Early_Universe|Cosmology]] |
[[http://dx.doi.org/10.1088/1475-7516/2020/03/050 Maggiore et al (2020)]] | [[http://dx.doi.org/10.1088/1475-7516/2020/03/050 Maggiore et al (2020)]] | ||
[[https://doi.org/10.1103/PhysRevD.102.022007 Grimm / Harms (2020)]] | [[https://doi.org/10.1103/PhysRevD.102.022007 Grimm / Harms (2020)]] | ||
Revision as of 17:07, 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.
