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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