Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements. Stegmann, J., Gerosa, D., Romero-Shaw, I., Fumagalli, G., Tagawa, H., & Zwick, L. arXiv, May, 2025.
bibtex   
@article{2025arXiv250513589S,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250513589S},
	archiveprefix = {arXiv},
	author = {{Stegmann}, Jakob and {Gerosa}, Davide and {Romero-Shaw}, Isobel and {Fumagalli}, Giulia and {Tagawa}, Hiromichi and {Zwick}, Lorenz},
	eid = {arXiv:2505.13589},
	eprint = {2505.13589},
	journal = {arXiv},
	keywords = {High Energy Astrophysical Phenomena, Solar and Stellar Astrophysics},
	month = may,
	pages = {arXiv:2505.13589},
	primaryclass = {astro-ph.HE},
	title = {{Distinguishing the origin of eccentric black-hole mergers with gravitational-wave spin measurements}},
	year = 2025}

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