Phys. Rev. D
76,
102001
(2007)
[9 pages]
Results of the IGEC-2 search for gravitational wave bursts during 2005
P. Astone et al. IGEC-2 Collaboration
Show All Authors/Affiliations
Hide All Authors/Affiliations
P. Astone1, D. Babusci2, L. Baggio3, M. Bassan4,5, M. Bignotto6,7, M. Bonaldi8,9, M. Camarda10, P. Carelli5,11, G. Cavallari12, M. Cerdonio6,7, A. Chincarini13, E. Coccia4,14, L. Conti6,7, S. D’Antonio5, M. De Rosa15,16, M. di Paolo Emilio11,14, M. Drago6,7, F. Dubath17, V. Fafone4,5, P. Falferi8,9, S. Foffa17, P. Fortini18, S. Frasca1,19, G. Gemme13, G. Giordano2, G. Giusfredi20, W. O. Hamilton21, J. Hanson21, M. Inguscio16,22, W. W. Johnson21, N. Liguori6,7, S. Longo23, M. Maggiore17, F. Marin16,22, A. Marini2, M. P. McHugh24, R. Mezzena9,25, P. Miller21, Y. Minenkov14, A. Mion9,25, G. Modestino2, A. Moleti4,5, D. Nettles21, A. Ortolan23, G. V. Pallottino1,19, R. Parodi13, G. Piano Mortari11,14, S. Poggi26, G. A. Prodi9,25,*, L. Quintieri2, V. Re9,25, A. Rocchi4, F. Ronga2, F. Salemi9,25, G. Soranzo7, R. Sturani17, L. Taffarello7, R. Terenzi1,27, G. Torrioli1,28, R. Vaccarone13, G. Vandoni12, G. Vedovato7, A. Vinante8,9, M. Visco4,27, S. Vitale9,25, J. Weaver21, J. P. Zendri7, and P. Zhang21 (IGEC-2 Collaboration)
1INFN, Sezione di Roma, Piazzale le A. Moro 2, I-00185, Roma, Italy 2INFN, Laboratori Nazionali di Frascati, Via E. Fermi 40, I-00044, Frascati, Italy 3EGO, 56021 Santo Stefano a Macerata, Cascina, Pisa, Italy 4Dipartimento di Fisica, Università di Roma “Tor Vergata,” Via Ricerca Scientifica 1, I-00133 Roma, Italy 5INFN, Sezione di Roma Tor Vergata, Via Ricerca Scientifica 1, I-00133 Roma, Italy 6Dipartimento di Fisica, Università di Padova, Via Marzolo 8, 35131 Padova, Italy 7INFN, Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy 8Istituto di Fotonica e Nanotecnologie, CNR-Fondazione Bruno Kessler, I-38050 Povo, Trento, Italy 9INFN, Gruppo Collegato di Trento, Sezione di Padova, I-38050 Povo, Trento, Italy 10Dipartimento di Ingegneria Informatica, Università di Padova, Via G. Gradenigo 6a, 35131 Padova, Italy 11Dipartimento di Fisica, Università de L’Aquila, L’Aquila, Italy 12CERN, Geneva, Switzerland 13INFN, Sezione di Genova, Genova, Italy 14INFN, Laboratori Nazionali del Gran Sasso, Assergi, L’Aquila, Italy 15INOA, CNR, I-80078 Pozzuoli, Napoli, Italy 16INFN, Sezione di Firenze, I-50121 Firenze, Italy 17Département de Physique Théorique, Université de Genève, Genève, Switzerland 18Dipartimento di Fisica, Università di Ferrara and INFN, Sezione di Ferrara, I-44100 Ferrara, Italy 19Dipartimento di Fisica, Università di Roma “La Sapienza,” Piazzale le A. Moro 2, I-00185, Roma, Italy 20INOA, CNR, I-50125 Arcetri, Firenze, Italy 21Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA 22LENS and Dipartimento di Fisica, Università di Firenze, I-50121 Firenze, Italy 23INFN, Laboratori Nazionali di Legnaro, 35020 Legnaro, Padova, Italy 24Department of Physics, Loyola University New Orleans, New Orleans, Louisiana 70118, USA 25Dipartimento di Fisica, Università di Trento, I-38050 Povo, Trento, Italy 26Consorzio Criospazio Ricerche, I-38050 Povo, Trento, Italy 27INAF, Istituto Fisica Spazio Interplanetario,Via Fosso del Cavaliere, I-00133 Roma, Italy 28CNR, Istituto di Fotonica e Nanotecnologie, Roma, Italy
Received 11 June 2007; published 1 November 2007
The network of resonant bar detectors of gravitational waves resumed coordinated observations within the International Gravitational Event Collaboration (IGEC-2). Four detectors are taking part in this Collaboration: ALLEGRO, AURIGA, EXPLORER and NAUTILUS. We present here the results of the search for gravitational wave bursts over 6 months during 2005, when IGEC-2 was the only gravitational wave observatory in operation. The implemented network data analysis is based on a time coincidence search among AURIGA, EXPLORER and NAUTILUS; ALLEGRO data was reserved for follow-up studies. The network amplitude sensitivity to bursts improved by a factor ≈3 over the 1997-2000 IGEC observations; the wider sensitive band also allowed the analysis to be tuned over a larger class of waveforms. Given the higher single-detector duty factors, the analysis was based on threefold coincidence, to ensure the identification of any single candidate of gravitational waves with high statistical confidence. The false detection rate was as low as 1 per century. No candidates were found.
© 2007 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevD.76.102001
DOI:
10.1103/PhysRevD.76.102001
PACS:
04.80.Nn, 95.30.Sf, 95.85.Sz
*Corresponding author. prodi@science.unitn.it
|
|