First joint gravitational wave search by the AURIGA-EXPLORER-NAUTILUS-Virgo Collaboration

被引：9

作者：

Acernese, F. ^{[1
,3
]}

Alshourbagy, M. ^{[4
,5
]}

Amico, P. ^{[8
,9
]}

Antonucci, F. ^{[11
]}

Aoudia, S. ^{[12
]}

Astone, P. ^{[11
]}

Avino, S. ^{[1
,2
]}

Babusci, D. ^{[13
]}

Baggio, L. ^{[14
]}

Ballardin, G. ^{[15
]}

Barone, F. ^{[1
,3
]}

Barsotti, L. ^{[4
,5
]}

Barsuglia, M. ^{[16
]}

Bassan, M. ^{[17
,18
]}

Bauer, Th S. ^{[20
]}

Bignotto, M. ^{[22
,23
]}

Bigotta, S. ^{[4
,5
]}

Birindelli, S. ^{[4
]}

Bizouard, M. A. ^{[16
]}

Boccara, C. ^{[2
]}

Bonaldi, M. ^{[24
,25
]}

Bondu, F. ^{[12
]}

Bosi, L. ^{[8
]}

Braccini, S. ^{[5
]}

Bradaschia, C. ^{[5
]}

Brillet, A. ^{[12
]}

Brisson, V. ^{[16
]}

Buskulic, D. ^{[14
]}

Cagnoli, G. ^{[26
]}

Calloni, E. ^{[1
,2
]}

Camarda, M. ^{[29
]}

Campagna, E. ^{[26
,28
]}

Carbognani, F.

Carelli, P. ^{[17
,19
]}

Cavalier, F. ^{[16
]}

Cavalieri, R. ^{[15
]}

Cavallari, G. ^{[30
]}

Cella, G. ^{[4
]}

Cerdonio, M. ^{[22
,23
]}

Cesarini, E. ^{[26
,27
]}

Chassande-Mottin, E. ^{[12
]}

Chincarini, A. ^{[31
]}

Clapson, A-C ^{[16
]}

Cleva, F. ^{[12
]}

Coccia, E. ^{[17
,18
]}

Conti, L. ^{[22
,23
]}

Corda, C. ^{[4
,5
]}

Corsi, A. ^{[11
]}

Cottone, F. ^{[8
,9
]}

Coulon, J-P

机构：

[1] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy

[2] Univ Naples Federico 2, Complesso Univ Monte S Angelo, Naples, Italy

[3] Univ Salerno, Fisciano, SA, Italy

[4] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy

[5] Univ Pisa, Pisa, Italy

[6] Scuola Normale Super Pisa, Pisa, Italy

[7] Univ Siena, I-53100 Siena, Italy

[8] Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy

[9] Univ Perugia, I-06100 Perugia, Italy

[10] Univ Roma La Sapienza, Rome, Italy

[11] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy

[12] Observ Cote Azur, CNRS, F-06304 Nice 4, France

[13] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy

[14] Univ Savoie, CNRS, IN2P3, Lab Annecy Le Vieux Phys Particules, Annecy Le Vieux, France

[15] EGO, Cascina, PI, Italy

[16] Univ Paris 11, CNRS, IN2P3, LAL, F-91405 Orsay, France

[17] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy

[18] Univ Roma Tor Vergata, Rome, Italy

[19] Univ Aquila, I-67100 Laquila, Italy

[20] Natl Inst Subatom Phys, NL-1009 DB Amsterdam, Netherlands

[21] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands

[22] Univ Padua, Dipartimento Fis, I-35131 Padua, Italy

[23] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[24] CNR Fdn Bruno Kessler, Ist Foton & Nanotecnol, I-38050 Trento, Italy

[25] Ist Nazl Fis Nucl, Grp Coll Trento, Sez Padova, I-38050 Trento, Italy

[26] Ist Nazl Fis Nucl, Sez Firenze, I-50125 Florence, Italy

[27] Univ Florence, Florence, Italy

[28] Univ Urbino Carlo Bo, Urbino, Italy

[29] Univ Padua, Dipartimento Ingn Informat, I-35131 Padua, Italy

[30] CERN, Geneva, Switzerland

[31] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy

[32] Univ Geneva, Dept Phys Theor, CH-1211 Geneva, Switzerland

[33] Univ Ferrara, Dipartmento Fis, I-44100 Ferrara, Italy

[34] Ist Nazl Fis Nucl, Sez Ferrara, I-44100 Ferrara, Italy

[35] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Padua, Italy

[36] ESPCI, F-75005 Paris, France

[37] CNRS, IN2P3, LMA, F-69622 Villeurbanne, Lyon, France

[38] Univ Trent, Dipartimento Fis, I-38050 Trento, Italy

[39] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila, Italy

[40] Consorzio Criospazio Ric, I-38050 Trento, Italy

[41] CNR, Ist Foton & Nanotecnol, Rome, Italy

[42] Ist Fis Spazio Interplanetario, INAF, Rome, Italy

来源：

CLASSICAL AND QUANTUM GRAVITY | 2008年 / 25卷 / 20期

关键词：

D O I：

10.1088/0264-9381/25/20/205007

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a methodology of network data analysis applied to the search for coincident burst excitations over a 24 h long data set collected by AURIGA, EXPLORER, NAUTILUS and Virgo detectors during September 2005. The search of candidate triggers was performed independently on each of the data sets from single detectors. We looked for two-fold time coincidences between these candidates using an algorithm optimized for a given population of sources and we calculated the efficiency of detection through injections of templated signal waveforms into the streams of data. To this end we have considered the case of signals shaped as damped sinusoids coming from the galactic center direction. Our method targets an optimal balance between high efficiency and low false alarm rate, aiming at setting confidence intervals as stringent as possible in terms of the rate of the selected source models.

引用

页数：20

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