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Table 3.

Summary of important coolants in our late-time magnetar-powered ejecta models. [See Section 4 for discussion.]

Ion Proc. Main lines
He I NT 3888.6 Å; 1.083, 2.058 μm
He II NT 4685.7 Å

C II COL 2325.4 Å
C II NT 1335.7, 6578.0–6582.9, 7231.3–7236.4 Å
C III COL 1906.7–1908.7 Å

N II COL 6548.0, 6583.4 Å

O I COL 6300.3, 6363.8 Å
O I NT 8446.4 Å
O II COL 3726.0–3728.8 Å
O II NT 7318.9, 7320.0, 7329.7, 7330.7 Å
O III COL 4958.9, 5006.8 Å
O III NT 4363.2 Å

Ne II COL 12.81 μm
Ne III COL 15.55 μm

Si II COL 1.691 μm
Si II NT 3856.0, 5056.0, 6347.1 Å
Si III COL 1882.7, 1892.0 Å

S I COL 25.242 μm
S II COL 6716.4 Å
S III COL 9068.6, 9530.6 Å; 18.708 μm

Ar II COL 6.983 μm
Ar III COL 7135.8 Å; 8.989, 21.826 μm

Fe I COL 24.036 μm
Fe II COL 17.931, 24.512, 25.981 μm
Fe III COL 4658.0, 5011.2 Å; 2.218, 7.788, 22.919 μm
Fe IV COL 2829.4, 2835.7 Å, 2.836 μm

Ni I COL 7.505 μm
Ni II COL 6.634, 10.679, 12.725 μm
Ni III COL 7.347, 10.999 μm

Notes. We list the ions and processes of relevance, together with the dominant associated lines. The list is ordered in increasing atomic number, and then in increasing ionization state, for all species. The term “COL” stands for collisional excitation and “NT” for nonthermal excitation.

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