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Future gravitational wave interferometers such as LISA, Taiji, DECIGO, and TianQin, will enable precision studies of the environment surrounding black holes.
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James Binney and Scott Tremaine, Galactic Dynamics: Second Edition (2008)
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Scott E. Field, Chad R. Galley, Frank Herrmann, Jan S. Hesthaven, Evan Ochsner, and Manuel Tiglio, “Reduced basis catalogs for gravitational wave templates,” Physical Review Letters 106
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Travis Robson, Neil J Cornish, and Chang Liu, “The construction and use of LISA sensitivity curves,” Classical and Quantum Gravity 36
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Bradley J. Kavanagh, “HaloFeedback [Code, v0.9],” https://github.com/bradkav/HaloFeedback , DOI:10.5281/zenodo.3688813 (2020)
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Chad R. Galley, “forked-rompy 0.03,” (2020)
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Ziren Luo, Yan Wang, Yueliang Wu, Wenrui Hu, and Gang Jin, “The Taiji program: A concise overview,” Progress of Theoretical and Experimental Physics 2021
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Lorenzo Speri and Jonathan R. Gair, “Assessing the impact of transient orbital resonances,” Phys. Rev. D 103
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Lorenzo Speri, Andrea Antonelli, Laura Sberna, Stanislav Babak, Enrico Barausse, Jonathan R. Gair, and Michael L. Katz, “Measuring accretion-disk effects with gravitational waves from extreme mass ratio inspirals,” (2022)
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Andrea Maselli, Nicola Franchini, Leonardo Gualtieri, Thomas P. Sotiriou, Susanna Barsanti, and Paolo Pani, “Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals,” Nature Astronomy 6
2022
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