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Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
Page(s) 603 - 604
Published online 15 September 1999
DOI: 10.1051/aas:1999370

Astron. Astrophys. Suppl. Ser. 138, 603-604

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

P. Astone1 - G. Barbiellini2 - M. Bassan3 - P. Bonifazi1,4 - P. Carelli6 - E. Coccia3,5 - V. Fafone5 - S. Frasca7 - F. Longo2 - E. Mauceli5 - Y. Minenkov3 - I. Modena3,5 - G. Modestino5 - A. Moleti3 - G.V. Pallottino1,7 - G. Pizzella3,5 - R. Terenzi1,4 - M. Visco1,4

Send offprint request: F. Longo:

1 - Istituto Nazionale di Fisica Nucleare (INFN), Roma, Italy
2 - University of Trieste and INFN, Trieste, Italy
3 - University of Roma "Tor Vergata" and INFN, Roma, Italy
4 - Istituto di Fisica dello Spazio Interplanetario, CNR, Roma, Italy
5 - Istituto Nazionale di Fisica Nucleare, Frascati, Italy
6 - University of L'Aquila and INFN, L'Aquila, Italy
7 - University of Roma "La Sapienza", Roma, Italy

Received December 18, 1998; accepted May 28, 1999


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 $\pm 5$ minutes around the trigger time of Gamma-Ray 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: $h \ge 2.5 \ 10^{-18}$.

Key words: gravitational waves -- gamma-ray: bursts

Copyright The European Southern Observatory (ESO)

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