Issue |
Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
|
|
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Page(s) | 605 - 606 | |
DOI | https://doi.org/10.1051/aas:1999371 | |
Published online | 15 September 1999 |
Measurements with the resonant gravitational wave detector EXPLORER during the gamma-ray burst 980425
1
Istituto di Astrofisica Spaziale, CNR, via Fosso del Cavaliere, Roma, Italy
2
Istituto Astronomico, University of Roma "La Sapienza”, via Lancisi 29, Roma, Italy
3
Istituto Nazionale di Fisica Nucleare (INFN), P.le A. Moro 2, Roma, Italy
4
University of Roma "Tor Vergata” and INFN, via O. Raimondo, Roma, Italy
5
Istituto di Fisica dello Spazio Interplanetario, CNR, via Fosso del Cavaliere, Roma, Italy
6
University of L'Aquila and INFN, via Vetoio (Coppito 1), Coppito di L'Aquila, Italy
7
Laboratori Nazionali di Frascati INFN, via E. Fermi 40, Frascati, Italy
8
University of Roma "La Sapienza”, P.le A. Moro 2, Roma, Italy
9
University of Ferrara, via Paradiso 12, Ferrara, Italy
10
Istituto TeSRE, CNR, via P. Gobetti 101, Bologna, Italy
11
University of Trieste and INFN, via A. Valerio 2, Trieste, Italy
Send offprint request to: P. Bonifazi
Received:
16
March
1999
Accepted:
5
July
1999
We report on the operation of the resonant gravitational wave (g.w.)
detector Explorer of the Rome group
( kg,
K,
located at CERN) at the time of the gamma-ray burst
GRB 980425 (April 25.90915 UT,
1998), which is probably associated with the supernova SN 1998bw.
We present the data of the detector (with
sensitivity
for a 1 ms
pulse), and use the BeppoSAX
data to estimate the initial time of the GRB:
a basic parameter for any correlation analysis.
The g.w. data exhibit no significant
time signature around the GRB 980425.
We wish to remark the importance
to make use, in spite of the present
low sensitivity, of the data collected with g.w.
detectors, that can be regarded as active observatories, in
coincidence with the BeppoSAX data.
Key words: gravitational waves / gamma-ray bursts
© European Southern Observatory (ESO), 1999