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Fig. 5.

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Examples of theoretical model fits with the observed abundances of the star. In panels a, b, and c, the points with error bars indicate the observed abundances. (a) s-process model fits for M = 1.3 M & 2.0 M. (b) i-process model fits for n = 1012 cm−3 and 1014 cm−3. (c) Best-fit from parametric-model. (d) Residual plot.

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