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Table 3.

Results for various linear combinations of nucleosynthetic processes in the fitting range of 31 ≤ Z ≤ 72.

Process(es) χ2 Notes Process(es) χ2 Notes
solar 154.72 1 sm2 + in9 66.31 3,2
in9 214.25 2 sm2 + in15 51.17 3,2
in10 229.76 2 sm5 + in9 59.25 5,2
in11 251.94 2 sm5 + in15 74.37 5,2
in12 257.21 2 Solar + in9 92.89 1,2
in13 304.40 2 Solar + in10 94.82 1,2
in14 463.06 2 Solar + in11 101.47 1,2
in15 539.71 2 Solar + in12 103.30 1,2
sm2 85.90 3 Solar + in13 109.14 1,2
sm3 63.56 4 Solar + in14 101.85 1,2
sm5 274.66 5 Solar + in15 94.44 1,2
sm3 + in9 63.15 4,2 sm3 + r + in9 63.00 4,6,2
sm3 + in10 62.94 4,2 sm3 + r + in10 62.80 4,6,2
sm3 + in11 62.77 4,2 sm3 + r + in11 62.72 4,6,2
sm3 + in12 61.23 4,2 sm3 + r + in12 61.23 4,6,2
sm3 + in13 59.95 4,2 sm3 + r + in13 59.92 4,6,2
sm3 + in14 59.71 4,2 sm3 + r + in14 59.71 4,6,2
sm3 + in15 54.97 4,2 sm3 + r + in15 54.57 4,6,2
sm3 + r 63.26 4,6 2-step i 50.96 7

Notes. References and model details: (1): Solar abundances from Lodders (2003); (2) i-process abundances from Hampel et al. (2016), using constant temperatures of T = 0.15 GK and constant densities of ρ = 1600 g cm−3. The respective neutron densities are indicated (as logN [cm−3]) by the subscript; (3): AGB yields for Minit = 2 M, Z = 0.0001 (Lugaro et al. 2012); (4): AGB yields for Minit = 3 M, Z = 0.0001 (Lugaro et al. 2012); (5): AGB yields for Minit = 5 M, Z = 0.0001 (Lugaro et al. 2012); (6): r-process from dynamical ejecta of binary neutron star merger (Korobkin et al. 2012); (7): i-process with two ingestion episodes of τ = 0.30 and 0.96 mbarn−1 (Sect. 5).

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