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AbstractAbstract
[en] The expected performances of the gravitational wave observatory composed by the five resonant detectors currently in operation are discussed. The potential near future improvements are also examined assuming that the noise properties of the up-graded resonant detectors will be in agreement with predictions. With the initial operation of long-baseline interferometers a substantial improvement in the burst search is expected
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Source
TAUP 97: 5. international workshop on topics in astroparticle and underground physics; L'Aquilla (Italy); 7-11 Sep 1997; S0920563298004903; Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Conference
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