Table 8
Strong lines observed in the post-outburst phase.
| Species | λ | References |
| (Å) | ||
|
|
||
| CrI: | 4078 | SA15 |
| FeII | 4351 | SA15 |
| Hβ | 4861 | SA12/SA15 |
| FeI/FeII | 4939/4924 | SA12/SA15 |
| FeII | 5018 | SA12/SA15 |
| FeI | 5027 | SA12 |
| FeI | 5050 | SA12 |
| FeI | 5056 | SA12 |
| FeI: | 5110 | SA12 |
| MgI | 5173 | SA15/SA12 |
| HeI | 5876 | SA15/SA12 |
| FeI/CrI | 6137/6138 | – |
| FeI: | 6180 | SA12 |
| FeI | 6355 | SA12/H14 |
| FeI | 6394 | SA12/H14 |
| FeI | 6426 | SA12/H14 |
| CaI/FeII | 6451/6456 | H14/SA12 |
| CaI | 6494 | H14/SA12 |
| FeII | 6516 | H14/SA12 |
| Hα | 6563 | SA12/SA15 |
| NiI/[NII]/CI | 6586/6583/6588 | SA12/H14/SA15 |
| FeII/HeI | 6679/6678 | H14/SA12/SA15 |
Notes. The laboratory wavelengths are given. Uncertain identifications are marked by “:”. Lines that have been observed in EX Lupi during outburst (SA12 Sicilia-Aguilar et al. 2012) or quiescence (SA15 Sicilia-Aguilar et al. 2015) and in the 2013 outburst of ASASSN-13db (H14 Holoien et al. 2014) are marked in the References column.
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