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51#
發(fā)表于 2025-3-30 09:07:31 | 只看該作者
https://doi.org/10.1007/978-1-4039-7003-9epresentative antennas and are seen to be operating near sensitivities allowing Galactic observations. Finally, each detector technology holds promises for increased sensitivity which will allow for collaborative detection of sources as distant as the Virgo cluster.
52#
發(fā)表于 2025-3-30 14:47:30 | 只看該作者
Coalescing Binaries to Post-Newtonian Orderpost-Newtonian amplitudes of the waves under the assumption that the detector is in the light-recycling configuration and that we use the matched filter technique to dig out the signal from the noise.
53#
發(fā)表于 2025-3-30 18:14:48 | 只看該作者
Comparison of Bars and Interferometers: Detection of Transient Gravitational Radiationepresentative antennas and are seen to be operating near sensitivities allowing Galactic observations. Finally, each detector technology holds promises for increased sensitivity which will allow for collaborative detection of sources as distant as the Virgo cluster.
54#
發(fā)表于 2025-3-30 20:42:57 | 只看該作者
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