Search for correlation between GRB's detected by BeppoSAX and gravitational wave detectors EXPLORER and NAUTILUS

被引:25
作者
Astone, P [1 ]
Bassan, M
Bonifazi, P
Carelli, P
Castellano, G
Coccia, E
Cosmelli, C
D'Agostini, G
D'Antonio, S
Fafone, V
Federici, G
Frontera, F
Guidorzi, C
Marini, A
Minenkov, Y
Modena, I
Modestino, G
Moleti, A
Montanari, E
Pallottino, GV
Pizzella, G
Quintieri, L
Rocchi, A
Ronga, F
Terenzi, R
Torrioli, G
Visco, M
机构
[1] Ist Nazl Fis Nucl, Rome, Italy
[2] Univ Roma Tor Vergata, Rome 2, Italy
[3] Ist Nazl Fis Nucl, Rome 2, Italy
[4] CNR, IFSI, Rome, Italy
[5] Univ Aquila, Rome 2, Italy
[6] CNR, IESS, Rome, Italy
[7] Univ Roma La Sapienza, Rome, Italy
[8] Ist Nazl Fis Nucl, Frascati, Italy
[9] CNR, IASF, I-40126 Bologna, Italy
[10] Univ Ferrara, Bologna, Italy
[11] Univ Ferrara, I-44100 Ferrara, Italy
[12] ITA I Calvi, Modena, Italy
[13] Univ Roma Tor Vergata, Frascati, Italy
[14] CNR, IFSI, Rome 2, Italy
[15] CNR, IFSI, Frascati, Italy
关键词
D O I
10.1103/PhysRevD.66.102002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Data obtained during five months of 2001 with the gravitational wave (GW) detectors EXPLORER and NAUTILUS, operating with a bandwidth of a few Hz at frequencies near 900 Hz, were studied in correlation with the gamma ray burst data (GRB) obtained with the BeppoSAX satellite. During this period BeppoSAX was the only GRB satellite in operation, while EXPLORER and NAUTILUS were the only GW detectors in operation. No correlation between the GW data and the GRB bursts was found. The analysis, performed over 47 GRB's, excludes the presence of signals of amplitude hgreater than or equal to6.5x10(-19), with 95% probability, if we allow a time delay between GW bursts and GRB within +/-5 s, and hgreater than or equal to1.2x10(-18), if the time delay is within +/-400 s. The result is also provided in the form of scaled likelihood for unbiased interpretation and easier use for further analysis.
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页数:8
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