Search for time correlation between gamma-ray bursts and data from the gravitational wave antenna EXPLORER

被引：12

作者：

Astone, P

Barbiellini, G

Bassan, M

Bonifazi, P

Carelli, P

Coccia, E

Fafone, V

Frasca, S

Longo, F ^{[1
]}

Mauceli, E

Minenkov, Y

Modena, I

Modestino, G

Moleti, A

Pallottino, GV

Pizzella, G

Terenzi, R

Visco, M

机构：

[1] Univ Trieste, Trieste, Italy

[2] Ist Nazl Fis Nucl, Trieste, Italy

[3] Ist Nazl Fis Nucl, Rome, Italy

[4] Univ Roma Tor Vergata, Rome, Italy

[5] CNR, Ist Fis Spazio Interplanetario, Rome, Italy

[6] Ist Nazl Fis Nucl, Frascati, Italy

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

[8] Ist Nazl Fis Nucl, I-67100 Laquila, Italy

[9] Univ Rome La Sapienza, Rome, Italy

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 138卷 / 03期

关键词：

gravitational waves; gamma-ray : bursts;

D O I：

10.1051/aas:1999370

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

An analysis of the time correlation between Gamma-Ray Bursts from BATSE detector and EXPLORER Gravitational Wave Antenna data was performed from april 1991 to december 1996. a time interval of +/-5 minutes around the trigger time of Gamma-Ragi Bursts (GRBs) was explored. No significant excess of coincidences between GRBs and EXPLORER events with an energy of about 100 mK was found. This result allows to exclude correlations with 1 ms Gravitational Wave (GW) bursts with amplitude: h greater than or equal to 2.5 10(-18).

引用

页码：603 / 604

页数：2

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