Table A.3
Model atoms used in CMFGEN calculations for the toy01 model.
Ion | NSL | Nfull | Last level | Nlines |
---|---|---|---|---|
Si II | 32 | 62 | 3s2 7g 2G | 1 032 |
Si III | 33 | 61 | 3s 5g3G | 615 |
Si IV | 37 | 48 | 10f 2Fo | 816 |
Si V | 1 | 1 | ||
S II | 56 | 324 | 3s 3p3(5So)4p 6P | 16965 |
S III | 48 | 98 | 3s 3p2(2D)3d 3P | 1 723 |
S IV | 27 | 67 | 3s 3p(3Po)4p 2D | 1 091 |
SV | 1 | 1 | ||
Ca II | 44 | 77 | 3p6 30w 2W | 3 365 |
Ca III | 16 | 40 | 3s2 3p5 5s 1Po | 210 |
Ca IV | 18 | 69 | 3s 3p5(3Po)3d 4Do | 646 |
Ca V | 1 | 1 | ||
Fe I | 44 | 136 | 3d6(5D)4s 4p x5Fo | 3 934 |
Fe II | 228 | 2698 | 3d5(4F)4s4pb4Go | 1 060 528 |
Fe III | 83 | 698 | 3d5(2H)4d 1K | 73 419 |
Fe IV | 100 | 1 000 | 3d4(3G)4f 4Po | 144005 |
Fe V | 47 | 191 | 3d3(4F)4d 5F | 7 892 |
Fe VI | 1 | 1 | ||
Co II | 44 | 162 | 3d6(5D)4s 4p 7Fo | 6 475 |
Co III | 33 | 220 | 3d6(3F)4p 4Do | 9836 |
Co IV | 27 | 164 | 3d5(4D)4p 3Fo | 5 759 |
Co V | 32 | 387 | 3d4(3F)4d 2H | 27 046 |
Co VI | 1 | 1 | ||
Ni II | 27 | 177 | 3d7(4P)4s 4p(3P) 4So | 5 757 |
Ni III | 20 | 107 | 3d7(2H)4p 3Io | 2 228 |
Ni IV | 20 | 130 | 3d6(3F2)4p 4Do | 3 375 |
Ni V | 46 | 183 | 3d5(2D3)4p 3Fo | 6033 |
Ni VI | 1 | 1 | ||
Total | 1068 | 7105 | 1 382750 |
Notes: Due to a gf cut (level dependent, gf > 10−4) only 377 383 lines were included in the non-LTE calculations of the level populations. 692 911 lines were include when computing the observed spectrum. Prior to 2.4 days post explosion a higher cut was used (gf > 10−3) in order to ease convergence. From 25.93 days onward we omitted the highest ionisation stages Fe V, Co V, and Ni V since their populations are too low to affect the radiative transfer.
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