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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