Results from LIGO's Second Search for Gravitational-Wave Bursts

Details Results from LIGO's Second Search for Gravitational-Wave Bursts Results from LIGO's Second Search for Gravitational-Wave Bursts

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..apr.v9003s&link_type=abstract

American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #V9.003

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Scientific paper

During 2003 the LIGO observatories completed their second data-taking run in search of gravitational waves. One class of signals sought is unmodeled gravitational-wave transients (``bursts'') of sub-second duration, such as might be produced by core-collapse supernovae or by the merger or ringdown of black holes. The methodology and results of the analysis for gravitational-wave bursts are presented, with emphasis on the techniques used to identify bursts and to estimate the sensitivity to astrophysical signals. Plans for future analyses are also outlined.

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