The WS4 nuclear mass model yields the best agreement with AME2020 masses and with observed heavy element abundances in eight r-process enhanced metal-poor stars, but the margin over the Duflo-Zuker model is small and lacks error bars.
& Martínez-Pinedo, G
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Impact of nuclear mass models on $r$-process nucleosynthesis and heavy element abundances in $r$-process enhanced metal-poor stars
The WS4 nuclear mass model yields the best agreement with AME2020 masses and with observed heavy element abundances in eight r-process enhanced metal-poor stars, but the margin over the Duflo-Zuker model is small and lacks error bars.