Calculations indicate low probabilities (up to 11% for 89Sr, 5% for 22Na) of COSI detecting gamma-ray lines from i-process isotopes in nearby post-AGB stars or white dwarfs.
Frontera, arXiv e-prints , arXiv:2502.10845 (2025), arXiv:2502.10845 [astro-ph.IM]
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Can COSI detect $\gamma$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?
Calculations indicate low probabilities (up to 11% for 89Sr, 5% for 22Na) of COSI detecting gamma-ray lines from i-process isotopes in nearby post-AGB stars or white dwarfs.