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Table 3
Approximate numbers of template light-curves (NLC) per variability class in the VVV Templates Project database, as of the time of writing.
| Variability class | NLC | |||||||
|
|
||||||||
| Cataclysmic variables (CV) | 5 | |||||||
| Classical Cepheids (DCEP) | 260 | |||||||
| Type-II Cepheids (CW) | 230 | |||||||
| Anomalous Cepheids (BLBOO) | 48 | |||||||
| Delta Scuti (DSCT) | 2 | |||||||
| Eclipsing binaries (EA+EB+EW) | 100 | |||||||
| Long-period variables (LPV) | 1000 | |||||||
| Orion variables (IN) | 1 | |||||||
| Quasi-stellar objects (QSO) | 70 | |||||||
| R Coronae Borealis (RCB) | 12 | |||||||
| RR Lyrae, type RRab (RRab) | 1600 | |||||||
| RR Lyrae, type RRc (RRc) | 90 | |||||||
| SX Phoenicis (SXPHE) | 9 | |||||||
| T Tauri stars (INT) | 1 | |||||||
| Wolf-Rayet stars (WR) | 6 | |||||||
| Young stellar objects (YSO) | 80 | |||||||
| X-ray binaries (X) | 2 | |||||||
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