Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..apr.r1019t&link_type=abstract
American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #R1.019
Astronomy and Astrophysics
Astrophysics
Scientific paper
The detection of radio wavelength transients from astrophysical sources can provide external triggers for gravitational wave (GW) searches within LIGO/Virgo data. There are a variety of sources of GWs that should also produce a radio transient, such as compact object inspirals and mergers, core- collapse super- novae, and the cusps or kinks of superconducting cosmic strings. Radio polarization and spectral information can help distinguish among candidate sources. Such a pulse may be detected by a transient radio array such as the Eight-meter-wavelength Transient Array (ETA). I will present details of an ongoing effort to perform a trans- spectral comparison between data from gravitational wave detectors and radio transient arrays. )
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