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Table A.1
The different variability classes considered by the current version of our supervised classification method.
| Stellar variability class | Abbreviation |
|
|
|
| β-Cephei stars | BCEP |
| Classical Cepheids | CLCEP |
| Double-mode Cepheids | DMCEP |
| δ-Scuti stars | DSCUT |
| Eclipsing binaries (all types) | ECL |
| Ellipsoidal variables | ELL |
| γ-Doradus stars | GDOR |
| Mira variables | MIRA |
| RR-Lyrae stars, subtype ab | RRAB |
| RR-Lyrae stars, subtype c | RRC |
| Double-mode RR-Lyrae stars | RRD |
| RV-Tauri stars | RVTAU |
| Slowly pulsating B-stars | SPB |
| Semi-regular variables | SR |
| Rotational modulation | ROT |
| Active stars | ACT |
| Miscellaneous | MISC |
Notes. The “Miscellaneous” category stands for objects not belonging to any of the variability classes we consider.
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