Coincidence analysis between periodic source candidates in C6 and C7 Virgo data

被引：15

作者：

Acernese, F. ^{[1
]}

Amico, P.

Alshourbagy, M.

Antonucci, F.

Aoudia, S.

Astone, P.

Avino, S.

Babusci, D.

Ballardin, G.

Barone, F.

Barsotti, L.

Barsuglia, M.

Bauer, Th S.

Beauville, F.

Bigotta, S.

Birindelli, S.

Bizouard, M. A.

Boccara, C.

Bondu, F.

Bosi, L.

Bradaschia, C.

Braccini, S.

van den Brand, F. J.

Brillet, A.

Brisson, V.

Buskulic, D.

Calloni, E.

Campagna, E.

Carbognani, F.

Cavalier, F.

Cavalieri, R.

Cella, G.

Cesarini, E.

Chassande-Mottin, E.

Christensen, N.

Corda, C.

Corsi, A.

Cottone, F.

Clapson, A-C

Cleva, F.

Coulon, J-P

Cuoco, E.

Dari, A.

Dattilo, V.

Davier, M.

del Prete, M.

De Rosa, R.

Di Fiore, L.

Di Virgilio, A.

Dujardin, B.

机构：

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

[2] Univ Naples Federico II, Naples, Italy

[3] Univ Salerno, Fisciano, SA, Italy

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

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

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

[7] Univ Pisa, I-56100 Pisa, Italy

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

[9] Univ Roma La Sapienza, Rome, Italy

[10] Observ Cote Azur, Dept Artemis, F-06304 Nice 4, France

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

[12] EGO, Cascina, PI, Italy

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

[14] NIKHEF, NL-1009 DB Amsterdam, Netherlands

[15] Free Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands

[16] Univ Savoie, CNRS, IN2P3, LAPP, Annecy Le Vieux, France

[17] ESPCI, F-75005 Paris, France

[18] Ist Nazl Fis Nucl, Sez Firenze Urbino, Sesto Fiorentino, Italy

[19] Univ Florence, I-50121 Florence, Italy

[20] Univ Urbino, I-61029 Urbino, Italy

[21] LMA, Lyon, France

来源：

CLASSICAL AND QUANTUM GRAVITY | 2007年 / 24卷 / 19期

关键词：

D O I：

10.1088/0264-9381/24/19/S12

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, we describe the analysis performed in the data of C6 and C7 commissioning runs of Virgo for the search of periodic sources of gravitational waves. The analysis is all-sky, covers the frequency range between 50 Hz and 1050 Hz and neutron star spin-down rate below 1.58 x 10(-8) Hz s(-1). Coincidences in the source parameter space between candidates found in the two data sets are required to reduce the false alarm probability. The procedure used to estimate the detection efficiency of the analysis pipeline, through the injection of simulated signals in the data, is also described.

引用

页码：S491 / S499

页数：9

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