Prospects for the detection of electromagnetic counterparts to gravitational wave events

Details Prospects for the detection of electromagnetic counterparts to gravitational wave events Prospects for the detection of electromagnetic counterparts to gravitational wave events

2003-03-22

arxiv.org/abs/astro-ph/0303512v1

Astrophys.J. 591 (2003) 1152-1156

Astronomy and Astrophysics

Astrophysics

5 pages, 1 table, 1 figure

Scientific paper

10.1086/375505

Various models for electromagnetic emissions correlated with the gravitational wave signals expected to be detectable by the current and planned gravitational wave detectors are studied. The position error on the location of a gravitational wave source is estimated, and is used to show that it could be possible to observe the electromagnetic counterparts to neutron star-neutron star or neutron star-black hole binary coalescences detected with the Advanced LIGO and the Virgo detectors.

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