Details
Originalsprache | Englisch |
---|---|
Seiten (von - bis) | 175-180 |
Seitenumfang | 6 |
Fachzeitschrift | Physics Letters, Section A: General, Atomic and Solid State Physics |
Jahrgang | 218 |
Ausgabenummer | 3-6 |
Publikationsstatus | Veröffentlicht - 5 Aug. 1996 |
Extern publiziert | Ja |
Abstract
We report an upper bound on the strain amplitude of gravitational wave bursts in a waveband from around 800 Hz to 1.25 kHz. In an effective coincident observing period of 62 hours, the prototype laser interferometric gravitational wave detectors of the University of Glasgow and Max Planck Institute for Quantum Optics, have set a limit of 4.9 × 10-16, averaging over wave polarizations and incident directions. This is roughly a factor of 2 worse than the theoretical best limit that the detectors could have set, the excess being due to unmodelled non-Gaussian noise. The experiment has demonstrated the viability of the kind of observations planned for the large-scale interferometers that should be on-line in a few years time.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Allgemeine Physik und Astronomie
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in: Physics Letters, Section A: General, Atomic and Solid State Physics, Jahrgang 218, Nr. 3-6, 05.08.1996, S. 175-180.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Results of the first coincident observations by two laser-interferometric gravitational wave detectors
AU - Nicholson, D.
AU - Dickson, C. A.
AU - Watkins, W. J.
AU - Schutz, B. F.
AU - Shuttleworth, J.
AU - Jones, G. S.
AU - Robertson, D. I.
AU - Mackenzie, N. L.
AU - Strain, K. A.
AU - Meers, B. J.
AU - Newton, G. P.
AU - Ward, H.
AU - Cantley, C. A.
AU - Robertson, N. A.
AU - Hough, J.
AU - Danzmann, K.
AU - Niebauer, T. M.
AU - Rüdiger, A.
AU - Schilling, R.
AU - Schnupp, L.
AU - Winkler, W.
PY - 1996/8/5
Y1 - 1996/8/5
N2 - We report an upper bound on the strain amplitude of gravitational wave bursts in a waveband from around 800 Hz to 1.25 kHz. In an effective coincident observing period of 62 hours, the prototype laser interferometric gravitational wave detectors of the University of Glasgow and Max Planck Institute for Quantum Optics, have set a limit of 4.9 × 10-16, averaging over wave polarizations and incident directions. This is roughly a factor of 2 worse than the theoretical best limit that the detectors could have set, the excess being due to unmodelled non-Gaussian noise. The experiment has demonstrated the viability of the kind of observations planned for the large-scale interferometers that should be on-line in a few years time.
AB - We report an upper bound on the strain amplitude of gravitational wave bursts in a waveband from around 800 Hz to 1.25 kHz. In an effective coincident observing period of 62 hours, the prototype laser interferometric gravitational wave detectors of the University of Glasgow and Max Planck Institute for Quantum Optics, have set a limit of 4.9 × 10-16, averaging over wave polarizations and incident directions. This is roughly a factor of 2 worse than the theoretical best limit that the detectors could have set, the excess being due to unmodelled non-Gaussian noise. The experiment has demonstrated the viability of the kind of observations planned for the large-scale interferometers that should be on-line in a few years time.
UR - http://www.scopus.com/inward/record.url?scp=0041374869&partnerID=8YFLogxK
U2 - 10.1016/0375-9601(96)00438-0
DO - 10.1016/0375-9601(96)00438-0
M3 - Article
AN - SCOPUS:0041374869
VL - 218
SP - 175
EP - 180
JO - Physics Letters, Section A: General, Atomic and Solid State Physics
JF - Physics Letters, Section A: General, Atomic and Solid State Physics
SN - 0375-9601
IS - 3-6
ER -