Cumulative analysis of the association between the data of the gravitational wave detectors NAUTILUS and EXPLORER and the gamma ray bursts detected by BATSE and BeppoSAX

被引：18

作者：

Astone, P

Babusci, D

Bassan, M

Carelli, P

Coccia, E

Cosmelli, C

D'Antonio, S

Fafone, V

Frontera, F

Giordano, G

Guidorzi, C

Marini, A

Minenkov, Y

Modena, I

Modestino, G

Moleti, A

Montanari, E

Pallottino, GV

Pizzella, G

Quintieri, L

Rocchi, A

Ronga, F

Sperandio, L

Terenzi, R

Torrioli, G

Visco, M

机构：

[1] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

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

[3] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[4] Ist Nazl Fis Nucl, Sez Roma 2, I-00133 Rome, Italy

[5] Univ Aquila, Dipartimento Fis, I-67010 Coppito, LAquila, Italy

[6] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Coppito, LAquila, Italy

[7] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy

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

[9] CNR, Ist Astrofis Spaziale & Fis Cosm, I-40129 Bologna, Italy

[10] ISA A Venturi, Modena, Italy

[11] CNR, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy

来源：

PHYSICAL REVIEW D | 2005年 / 71卷 / 04期

关键词：

D O I：

10.1103/PhysRevD.71.042001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The statistical association between the output of the Gravitational Wave (GW) detectors EXPLORER and NAUTILUS and a list of Gamma Ray Bursts (GRBs) detected by the satellite experiments BATSE and BeppoSAX has been analyzed using cumulative algorithms. GW detector data collected between 1991 and 1999 have been searched for an energy excess in a 10 s interval around the GRB flux peak times. The cumulative analysis of the data relative to a large number of GRBs (387) allows to push the upper bound for the corresponding GW burst amplitude down to h=2.5x10(-19).

引用

页码：042001 / 1

页数：6

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