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Table A.3.
Acronyms used in the remark column of TableA.1.
| Acronym | Explanation |
|---|---|
| AALs | associated absorption lines |
| AsBLs | asymmetric broad Balmer lines |
| CyHs | cyclotron humps in stellar spectrum |
| DBR | displacement between blue and red part |
| DLAS | damped Lyα system |
| DLs | double narrow emission lines |
| DPBLs | double-peaked broad Balmer lines |
| Fe-em | strong Fe II emission |
| FeIII-em | strong FeIII emission |
| GP | possibly Gunn-Petterson trough |
| HBD | high Balmer decrement |
| IALs | intermediate absorption lines |
| Lya abs | Lyα line significantly absorbed |
| MATs | many absorption troughs |
| NBO | bright object nearby |
| NBS | blue part dominated by nearby blue source |
| NERP | non-genuine emission peak near red edge |
| PM | significant proper motion (Gaia DR3) |
| PSB | post-starburst |
| red | unusually red continuum |
| RWA | red wing of emission line absorbed |
| SELs | star with remarkably strong emission lines |
| sLya | very strong Lyα emission line |
| UC | unusual continuum |
| unusual | spectral type identified, but unusual |
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