Results 151 to 160 of about 138,364 (279)
Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer
The Astrophysical Journal LettersAccreting main-sequence stars expand significantly when the mass accretion timescale is much shorter than their thermal timescales. This occurs during mass transfer from an evolved giant star onto a main-sequence companion in a binary system and is an ...
Mike Y. M. Lau +3 more
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TechnologiesSpace-based gravitational wave detection relies on laser interferometry to measure picometer-level displacements over 105–106 km baselines. To integrate ranging and communication within the same optical link without degrading the primary scientific ...
Hongling Ling +3 more
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Growing Pains: Understanding the Impact of Likelihood Uncertainty on Hierarchical Bayesian Inference for Gravitational-Wave Astronomy [PDF]
, 2023 C. Talbot, Jacob Golomb
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Choosing Suitable Noise Models for Nanohertz Gravitational-wave Astrophysics
The Astrophysical JournalAccurately estimating the parameters of the nanohertz gravitational-wave background is essential for understanding its origin. The background is typically modeled with a power-law spectrum, parameterized with an amplitude A , which describes its ...
Valentina Di Marco +4 more
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Towards gravitational wave astronomy: Commissioning and characterization of GEO600
, 2006 S. Hild +4 more
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Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays
, 2018 Yan Wang, Soumya D. Mohanty
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GRAVITATIONAL WAVES AND ASTRONOMY [PDF]
Publications of The Korean Astronomical Society, 2011 Hyung-Mok Lee +5 more
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Solar Plasma Noise in TianQin Laser Propagation: An Extreme Case and Statistical Analysis
The Astrophysical JournalTianQin (TQ) proposes to detect gravitational-wave signals by using laser interferometry. However, the laser propagation effect introduces a potential noise factor for TQ.
Yanan Liu +4 more
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