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Table A.1

Times over which specific optical electron-scattering broadened emission lines are present in the model spectra computed for our 27 ejecta and CSM configurations characterized by different values of Ekin, Ṁ, and Rcsm.

Ekin [foe] M.[ Myr1 ]Mathematical equation: $\mathop {\rm{M}}\limits^. \left[ {{M_ \odot }{\rm{y}}{{\rm{r}}^{ - 1}}} \right]$ RCSM [1014 cm] IIn phase He 15875.66Å He ii 4685.70Å C iii 5695.92Å C iv 5804.86Å “N iii-C iii N iv 7109.35Å N v 4612.72Å O v 5597Å O vi 3820Å
0.6 0.001 2 ≤2.1 [0.3-1.7] [0.8-13] [1.0-1.7] [0.8-1.2] [0.6-0.7] 0.3∕0.7 0.5
0.6 0.001 6 ≤3.8 [0.3-2.3] [1.5-2.2] [0.7-1.2] [1.0-2.0] [0.8-1.0] 0.6 0.6 0.5
0.6 0.001 10 ≤5.2 [0.5-2.0] [0.5-1.0] [1.0-2.0] [0.8-1.0] [0.5-0.7] [0.5-0.7] 0.5

0.6 0.01 2 ≤3.2 [0.6-3.0] 0.6∕[2.0-2.5] 0.6∕2.5 0.6∕[2.0-2.5] [1.0-2.0] [1.0-1.7] [1.0-1.4]
0.6 0.01 6 ≤8.8 [4.0-6.7] [1.0-6.7] [4.0-6.7] [1.3-3.5] 1.0∕[3.3-5.0] [L3-3.3] 2.0
0.6 0.01 10 >15.0 1.3∕[4.0-12.0] [1.3-6.0] [5.0-7.0] [1.7-3.3] [1.3-6.0]

0.6 0.1 2 ≤4.7 2.0 [2.0-4.5] 2.0 2.2∕[3.8-4.3] [2.0-2.3] [2.0-2.4]∕[3.8-4.3] [2.3-3.8] [2.3-3.5]∕3.3 [2.6-3.3]
0.6 0.1 6 ≤14.9 [4.2-5.0]∕[11.5-13.3] [5.0-11.5] 5.0/11.5 [5.8-10.0] [5.0-11.5] [5.8-10.0] 5.8∕7.5 [7.5-9.0]
0.6 0.1 10 >15.0 [6.0-10.0] [10.0-15.0] [10.0-15.0] [11.6-15.0] 10.0-15.0]


1.2 0.001 2 ≤1.4 [03-1.4] [0.7-1.3] [0.8-1.2] [0.5-0.7] [0.5-0.7] 0.5
1.2 0.001 6 ≤2.7 [0.3-2.7] [1.6-2.3] [0.8-1.2] [1.0-2.0] [0.7-1.2] [0.5-0.7] [0.5-0.7] 0.5
1.2 0.001 10 ≤3.7 [0.3-2.7] [0.8-1.2] [1.0-2.5] [0.8-1.0] [0.5-0.8] [0.5-0.8] 0.5

1.2 0.01 2 ≤2.3 [0.5-2.2] [0.5-1.7]∕[1.5-2.2] 0.5∕[2.0-2.2] 0.7∕[1.8-2.2] [0.7-1.7] [0.8-L 刀 [1.0-1.4]
1.2 0.01 6 ≤6.3 [0.7-0.8]∕[5.0-6.0] [0.7-5.5] [5.0-5.5] [1.2-3.3] 0.8∕[3.3-5.0] [1.2-3.3] 1.7
1.2 0.01 10 ≤11.7 1.2∕[5.0-10.0] [1.2-6.7] [5.0-7.0] [L3-3.3] [33-5.0] [1.7-3.3]

1.2 0.1 2 ≤3.2 1.5 [1.8-3.0] [3.0-3.3] 1.5 [32-3.3] 1.8∕[2.6-3.0] 1.8∕[2.6-3.0] [1.8-2.7]
1.2 0.1 6 ≤10.9 4.2/10.0 [4.2-10.0] 4.2/10.0 [5.0-8.3] 4.2∕[8.3-9.2] 5.0∕[7.5-8.3] [5.0-6.7] [5.0-7.5] 5.8
1.2 0.1 10 >15.0 [5.0-6.7] [6.7-15.0] 6.7 [7.5-13.3] [6.7-15.0] [8.3-13.3]


1.8 0.001 2 ≤1.1 [0.1-1.0] [0.6-0.8] [0.6-1.0] [0.6-1.0] [0.5-0.7] [0.5-0.7] 0.3
1.8 0.001 6 ≤2.1 [0.3-2.0] 0.8 [0.7-1.2] [1.2-2.0] [0.7-0.8] [0.5-0.7] [0.5-0.7] [0.3-0.5]
1.8 0.001 10 ≤2.9 [0.3-2.0] [0.7-1.0] [1.0-2.5] [0.7-1.0] [0.5-0.7] [0.5-0.7] 0.3

1.8 0.01 2 ≤1.8 [0.5-1.7] [1.5-1.8] [1.7-1.8] [0.5-1.5] 0.5∕[1.3-1.5] [0.5-1.2]
1.8 0.01 6 ≤5.0 [L2-5.0] [1.2-3.3] [3.3-4.2] [2.0-3.3] [1.2-2.0] [1.2-3.3] 1.5
1.8 0.01 10 ≤9.4 [5.0-9.0] [1.3-7.5] [5.0-7.5] [1.3-4.2] [2.5-8.3] [L3-3.3] [1.3-2.0]

1.8 0.1 2 ≤2.5 [13-2.3] 1.3∕2.7 1.3 1.3 2.3 [1.7-2.0]
1.8 0.1 6 ≤8.6 [3.3-8.3] 8.3 [3.3-7.5] 3.3∕[7.5-8.3] [6.7-7.5] [4.2-5.8] 4.2∕5.8 5.0
1.8 0.1 10 >15.0 5.0/15.0 [6.7-15.0] [13.0-15.0] [6.7-13.3] [10.0-15.0] [6.7-11.7] [8.3-10.0] [8.3-10.0]

Notes: All times (or epochs) are in days since the SN shock crosses R* in the HERACLES simulation. NIII-C III” corresponds to the blend of multiplets due to both N III and C III and in particular N III 4640.64 Å and C III 4647.42 Å. [a –b]” means that a given line is present between epochs a and b. a∕b” means that the line was present at time a and time b, but not in between. A single quoted epoch implies the corresponding line was present in only one of the computed spectra (and thus absent before and after).

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