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Plans for the LIGO-TAMA Joint Search for Gravitational Wave Bursts
General Relativity and Quantum Cosmology · Submitted 28 Dec 2004
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We describe the plans for a joint search for unmodelled gravitational wave bursts being carried out by the LIGO and TAMA collaborations using data collected during February-April 2003.
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The abstract, sentence by sentence
We describe the plans for a joint search for unmodelled gravitational wave bursts being carried out by the LIGO and TAMA collaborations using data collected during February-April 2003. We take a conservative approach to detection, requiring candidate gravitational wave bursts to be seen in coincidence by all four interferometers. We focus on some of the complications of performing this coincidence analysis, in particular the effects of the different alignments and noise spectra of the interferometers.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We describe the plans for a joint search for unmodelled gravitational wave bursts being carried out by the LIGO and TAMA collaborations using data collected during February-April 2003. | contribution 0.98 | 0.80 | 0.12 | asserted 0.98 |
| s1 | We take a conservative approach to detection, requiring candidate gravitational wave bursts to be seen in coincidence by all four interferometers. | method 0.99 | 0.64 | 0.10 | asserted 0.98 |
| s2 | We focus on some of the complications of performing this coincidence analysis, in particular the effects of the different alignments and noise spectra of the interferometers. | method 0.58 | 0.41 | 0.06 | asserted 0.81 |
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The paper
Original abstract
We describe the plans for a joint search for unmodelled gravitational wave bursts being carried out by the LIGO and TAMA collaborations using data collected during February-April 2003. We take a conservative approach to detection, requiring candidate gravitational wave bursts to be seen in coincidence by all four interferometers. We focus on some of the complications of performing this coincidence analysis, in particular the effects of the different alignments and noise spectra of the interferometers.
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