Fig. 15: $P_n$ Sensitivity Studies Table

Important nuclei from the delayed neutron emission sensitivity studies of Fig. 15 given criterion $F_{max} \ge 0.1$ for at least one astrophysical condition: (a) low entropy hot wind, (b) high entropy hot wind, (c) cold wind and (d) neutron star merger. Asterisk denotes $F_{max}$ below threshold of $0.01$.
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Nucleus $P_n$
Z N A $F^a_{max}$ $F^b_{max}$ $F^c_{max}$ $F^d_{max}$