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樓主: Deleterious
61#
發(fā)表于 2025-4-1 03:57:36 | 只看該作者
Prologue Napoleon and the French Revolution,e show some preliminary results in the context of an array of optical telescopes called BlackGEM, dedicated for optical follow-up of GW triggers, that is being constructed in La Silla, Chile and is expected to operate concurrent to the advanced GW detectors.
62#
發(fā)表于 2025-4-1 08:52:09 | 只看該作者
63#
發(fā)表于 2025-4-1 13:03:54 | 只看該作者
Kleist als Dichter des Widerstands,e used in low-latency data analysis to restrict the parameter space searching for gravitational signals associated with short gamma-ray bursts, and to gain information on the dynamics of the coalescing system and on the neutron star equation of state.
64#
發(fā)表于 2025-4-1 15:21:43 | 只看該作者
65#
發(fā)表于 2025-4-1 19:12:10 | 只看該作者
https://doi.org/10.1007/978-3-319-60330-8oise ratios?~?10, typical of those expected for the first detections with Advanced LIGO/Virgo. Spin-orbit resonances thus consist in powerful, viable, probes of astrophysical processes in stellar-mass black-hole binary formation and evolution.
66#
發(fā)表于 2025-4-2 01:00:25 | 只看該作者
67#
發(fā)表于 2025-4-2 04:19:47 | 只看該作者
X, Gamma-Rays, and Gravitational Waves Emission in a Short Gamma-Ray Burst,?2?Gpc. We assess the detectability of this source by the Advanced LIGO interferometer computing the signal-to-noise ratio (SNR) averaged over all polarizations and possible positions of the source with respect to the interferometer. We simulate the dynamics of the binary up to the contact point usi
68#
發(fā)表于 2025-4-2 09:05:52 | 只看該作者
Localizing Gravitational Wave Sources with Optical Telescopes and Combining Electromagnetic and Grae show some preliminary results in the context of an array of optical telescopes called BlackGEM, dedicated for optical follow-up of GW triggers, that is being constructed in La Silla, Chile and is expected to operate concurrent to the advanced GW detectors.
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