A Joint Search for Gravitational Wave Bursts with AURIGA and LIGO
AURIGA Collaboration, LIGO Scientific Collaboration: L. Baggio et al

TL;DR
This paper presents the first joint search for gravitational wave bursts using AURIGA's resonant bar detector and LIGO's interferometers, focusing on methodology and setting upper limits in the absence of detection.
Contribution
It introduces a novel joint analysis method combining resonant and interferometric detectors and discusses the first unified approach between these different gravitational wave detection communities.
Findings
No gravitational wave bursts detected in the analyzed data.
Established a methodology for joint analysis of different detector types.
Set upper limits on gravitational wave event rates.
Abstract
The first simultaneous operation of the AURIGA detector and the LIGO observatory was an opportunity to explore real data, joint analysis methods between two very different types of gravitational wave detectors: resonant bars and interferometers. This paper describes a coincident gravitational wave burst search, where data from the LIGO interferometers are cross-correlated at the time of AURIGA candidate events to identify coherent transients. The analysis pipeline is tuned with two thresholds, on the signal-to-noise ratio of AURIGA candidate events and on the significance of the cross-correlation test in LIGO. The false alarm rate is estimated by introducing time shifts between data sets and the network detection efficiency is measured with simulated signals with power in the narrower AURIGA band. In the absence of a detection, we discuss how to set an upper limit on the rate of…
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