Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes. Fumagalli, G., Romero-Shaw, I., Gerosa, D., De Renzis, V., Kritos, K., & Olejak, A. Physical Review D, 110(6):063012, September, 2024.
doi  bibtex   
@article{2024PhRvD.110f3012F,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2024PhRvD.110f3012F},
	archiveprefix = {arXiv},
	author = {{Fumagalli}, Giulia and {Romero-Shaw}, Isobel and {Gerosa}, Davide and {De Renzis}, Viola and {Kritos}, Konstantinos and {Olejak}, Aleksandra},
	doi = {10.1103/PhysRevD.110.063012},
	eid = {063012},
	eprint = {2405.14945},
	journal = {Physical Review D},
	keywords = {Astrophysics and astroparticle physics, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = sep,
	number = {6},
	pages = {063012},
	primaryclass = {astro-ph.HE},
	title = {{Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes}},
	volume = {110},
	year = 2024,
	bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.110.063012}}

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