Authors

P. Astone, Istituto Nazionale di Fisica Nucleare - INFN
L. Baggio, CNRS Centre National de la Recherche Scientifique
M. Bassan, Università degli Studi di Roma "Tor Vergata"
M. Bignotto, Università degli Studi di Padova
M. Bonaldi, Bruno Kessler Foundation
P. Bonifazi, Istituto Nazionale di Fisica Nucleare - INFN
G. Cavallari, European Organization for Nuclear Research
M. Cerdonio, Università degli Studi di Padova
E. Coccia, Università degli Studi di Roma "Tor Vergata"
L. Conti, Istituto Nazionale Di Fisica Nucleare, Sezione di Padova
S. D'Antonio, Istituto Nazionale di Fisica Nucleare - INFN
M. Di Paolo Emilio, Laboratori Nazionali del Gran Sasso
M. Drago, Università degli Studi di Padova
V. Fafone, Università degli Studi di Roma "Tor Vergata"
P. Falferi, Bruno Kessler Foundation
S. Foffa, Université de Genève
P. Fortini, University of Ferrara
S. Frasca, Istituto Nazionale di Fisica Nucleare - INFN
G. Giordano, INFN, Laboratori Nazionali Di Frascati
W. O. Hamilton, Louisiana State University
J. Hanson, Louisiana State University
W. W. Johnson, Louisiana State University
N. Liguori, Università degli Studi di Padova
S. Longo, Istituto Nazionale Di Fisica Nucleare, Sezione di Padova
M. Maggiore, Université de Genève
F. Marin, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
A. Marini, INFN, Laboratori Nazionali Di Frascati
M. P. McHugh, Loyola University New Orleans
R. Mezzena, Trento Institute for Fundamental Physics and Applications
P. Miller, Louisiana State University
Y. Minenkov, Laboratori Nazionali del Gran Sasso
A. Mion, Trento Institute for Fundamental Physics and Applications
G. Modestino, INFN, Laboratori Nazionali Di Frascati

Document Type

Article

Publication Date

7-15-2010

Abstract

We present here the results of a 515 day search for short bursts of gravitational waves by the IGEC2 observatory. This network included 4 cryogenic resonant-bar detectors: AURIGA, EXPLORER, and NAUTILUS in Europe, and ALLEGRO in America. These results cover the time period from November 6th 2005 until April 15th 2007, partly overlapping the first long term observations by the LIGO interferometric detectors. The observatory operated with high duty cycle, namely, 57% for fourfold coincident observations, and 94% for threefold observations. The sensitivity was the best ever obtained by a bar network: we could detect, with an efficiency >50%, impulsive events with a burst strain amplitude hrss1×10-19Hz-1/2. The network data analysis was based on time coincidence searches over at least three detectors, used a blind search technique, and was tuned to achieve a false alarm rate of 1/century. When the blinding was removed, no gravitational wave candidate was found. © 2010 The American Physical Society.

Publication Source (Journal or Book title)

Physical Review D - Particles, Fields, Gravitation and Cosmology

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