Search for Gravitational-wave Inspiral Signals Associated with Short Gamma-ray Bursts During Ligo’s Fifth and Virgo’s First Science Run
Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by the emission of strong gravitational waves. We present a search for these known gravitational-wave signatures in temporal...
| Autores principales: | , , , , , , , , , , , , , , , , , |
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| Otros Autores: | |
| Formato: | Artículo |
| Lenguaje: | en_US |
| Publicado: |
IOP Publishing
2013
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| Acceso en línea: | http://hdl.handle.net/1721.1/76674 https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0001-7616-7809 https://orcid.org/0000-0001-8166-6805 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0003-1983-3187 |
| Sumario: | Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by the emission of strong gravitational waves. We present a search for these known gravitational-wave signatures in temporal and directional coincidence with 22 GRBs that had sufficient gravitational-wave data available in multiple instruments during LIGO's fifth science run, S5, and Virgo's first science run, VSR1. We find no statistically significant gravitational-wave candidates within a [ – 5, + 1) s window around the trigger time of any GRB. Using the Wilcoxon-Mann-Whitney U-test, we find no evidence for an excess of weak gravitational-wave signals in our sample of GRBs. We exclude neutron star-black hole progenitors to a median 90% confidence exclusion distance of 6.7 Mpc. |
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