Sequential simulation-based inference for extreme mass ratio inspirals. Cole, P. S., Alvey, J., Speri, L., Weniger, C., Bhardwaj, U., Gerosa, D., & Bertone, G. arXiv, May, 2025.
doi  bibtex   
@article{2025arXiv250516795C,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250516795C},
	archiveprefix = {arXiv},
	author = {{Cole}, Philippa S. and {Alvey}, James and {Speri}, Lorenzo and {Weniger}, Christoph and {Bhardwaj}, Uddipta and {Gerosa}, Davide and {Bertone}, Gianfranco},
	doi = {10.48550/arXiv.2505.16795},
	eid = {arXiv:2505.16795},
	eprint = {2505.16795},
	journal = {arXiv},
	keywords = {General Relativity and Quantum Cosmology, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics},
	month = may,
	pages = {arXiv:2505.16795},
	primaryclass = {gr-qc},
	title = {{Sequential simulation-based inference for extreme mass ratio inspirals}},
	year = 2025,
	bdsk-url-1 = {https://doi.org/10.48550/arXiv.2505.16795}}

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