IGEC2: A 17-month search for gravitational wave bursts in 2005-2007
P. Astone, L. Baggio, M. Bassan, M. Bignotto, M. Bonaldi, P. Bonifazi,, M. Cerdonio, E. Coccia, L. Conti, S. D'Antonio, M. di Paolo Emilio, M. Drago,, V. Fafone, P. Falferi, S. Foffa, P. Fortini, S. Frasca, G. Giordano, W.O., Hamilton, J. Hanson, W.W. Johnson, N. Liguori

TL;DR
This paper reports on a 17-month search for gravitational wave bursts using four resonant mass detectors, achieving high duty cycles and low false alarm rates, but finding no gravitational wave candidates.
Contribution
First long-term multi-detector search for gravitational wave bursts with resonant mass detectors, establishing a methodology and setting upper limits on event rates.
Findings
No gravitational wave candidates detected.
Achieved a false alarm rate of 1 per century.
Maintained high duty cycle with 57% with all four detectors.
Abstract
We present here the results of a 515 days long run of the IGEC2 observatory, consisting of the four resonant mass detectors ALLEGRO, AURIGA, EXPLORER and NAUTILUS. The reported results are related to the fourfold observation time from Nov. 6 2005 until Apr. 14 2007, when Allegro ceased its operation. This period overlapped with the first long term observations performed by the LIGO interferometric detectors. The IGEC observations aim at the identification of gravitational wave candidates with high confidence, keeping the false alarm rate at the level of 1 per century, and high duty cycle, namely 57% with all four sites and 94% with at least three sites in simultaneous observation. The network data analysis is based on time coincidence searches over at least three detectors: the four 3-fold searches and the 4-fold one are combined in a logical OR. We exchanged data with the usual blind…
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