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Fig. 13.
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Evolution of estimated NS merger rates in the Milky Way based on observable Galactic binaries during the last two decades, quoting the 90% or 95% confidence intervals (Kim et al. 2003, 2010, 2015; Kalogera et al. 2004; Pol et al. 2019, 2020; Grunthal et al. 2021).
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