GW200208_222617 as an eccentric black-hole binary merger: Properties and astrophysical implications. Romero-Shaw, I., Stegmann, J., Tagawa, H., Gerosa, D., Samsing, J., Gupte, N., & Green, S. R. \prd, 112(6):063052, September, 2025. doi bibtex @article{2025PhRvD.112f3052R,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025PhRvD.112f3052R},
archiveprefix = {arXiv},
author = {{Romero-Shaw}, Isobel and {Stegmann}, Jakob and {Tagawa}, Hiromichi and {Gerosa}, Davide and {Samsing}, Johan and {Gupte}, Nihar and {Green}, Stephen R.},
doi = {10.1103/jj7m-x66y},
eid = {063052},
eprint = {2506.17105},
journal = {\prd},
keywords = {Astrophysics and astroparticle physics, High Energy Astrophysical Phenomena, Astrophysics of Galaxies, General Relativity and Quantum Cosmology, High Energy Physics - Theory},
month = sep,
number = {6},
pages = {063052},
primaryclass = {astro-ph.HE},
title = {{GW200208\_222617 as an eccentric black-hole binary merger: Properties and astrophysical implications}},
volume = {112},
year = 2025,
bdsk-url-1 = {https://doi.org/10.1103/jj7m-x66y}}
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