Where did heavy binaries go? Gravitational-wave populations using Delaunay triangulation with optimized complexity. Tenorio, R., Toubiana, A., Bruel, T., Gerosa, D., & Gair, J. R. arXiv e-prints, September, 2025.
bibtex   
@article{2025arXiv250919466T,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250919466T},
	archiveprefix = {arXiv},
	author = {{Tenorio}, Rodrigo and {Toubiana}, Alexandre and {Bruel}, Tristan and {Gerosa}, Davide and {Gair}, Jonathan R.},
	eid = {arXiv:2509.19466},
	eprint = {2509.19466},
	journal = {arXiv e-prints},
	keywords = {High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = sep,
	pages = {arXiv:2509.19466},
	primaryclass = {astro-ph.HE},
	title = {{Where did heavy binaries go? Gravitational-wave populations using Delaunay triangulation with optimized complexity}},
	year = 2025}

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