Bayesian Inference for Gravitational Waves from Binary Neutron Star Mergers in Third Generation Observatories

Third generation (3G) gravitational-wave detectors will observe thousands of coalescing neutron star binaries with unprecedented fidelity. Extracting the highest precision science from these signals is expected to be challenging owing to both high signal-to-noise ratios and long-duration signals. We...

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Main Authors: Smith, Rory, Borhanian, Ssohrab, Sathyaprakash, Bangalore, Hernandez Vivanco, Francisco, Field, Scott E, Lasky, Paul, Mandel, Ilya, Morisaki, Soichiro, Ottaway, David, Slagmolen, Bram JJ, Thrane, Eric, Töyrä, Daniel, Vitale, Salvatore
מחברים אחרים: Massachusetts Institute of Technology. Department of Physics
פורמט: Article
שפה:English
יצא לאור: American Physical Society (APS) 2022
גישה מקוונת:https://hdl.handle.net/1721.1/142300

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