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Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
Carl-Johan Haster, Zhilu Wang, Christopher P. L. Berry +3
Gravitational waves from coalescences of neutron stars or stellar-mass black holes into intermediate-mass black holes (IMBHs) of solar masses represent one of the exc…
Parameter estimation on gravitational waves from neutron-star binaries with spinning components
Ben Farr, Christopher P. L. Berry, Will M. Farr +14
Inspiraling binary neutron stars are expected to be one of the most significant sources of gravitational-wave signals for the new generation of advanced ground-based detectors. We…
Planned search for LIGO-GBM coincidence in the first advanced LIGO data run
Jordan Camp, Lindy Blackburn, Michael Briggs +5
In the fall of 2015 the first scientific observing run (O1) of the advanced LIGO detectors will be conducted. Based on the recent commissioning progress at the LIGO Hanford and Liv…
Measuring intermediate mass black hole binaries with advanced gravitational wave detectors
John Veitch, Michael Pürrer, Ilya Mandel
We perform a systematic study to explore the accuracy with which the parameters of intermediate-mass black-hole binary systems can be measured from their gravitational wave (GW) si…
Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars
Michalis Agathos, Jeroen Meidam, Walter Del Pozzo +5
Recently exploratory studies were performed on the possibility of constraining the neutron star equation of state (EOS) using signals from coalescing binary neutron stars, or neutr…