Table 1
Stellar variability classes with high-quality IR time-series data from the literature, the GCVS designation (in brackets), the number of retrieved light-curves (NLC), and the corresponding reference source(s).
| Variability class | NLC | References | ||||||
|
|
||||||||
| Cataclysmic variables (CV) | 4 | Szkody et al. (1983); Bailey et al. (1985); Ribeiro & Baptista (2011) | ||||||
| Classical Cepheids (DCEP) | ~240 | P04; G13; MP11; R12(a, b); M14a | ||||||
| Anomalous Cepheids (BLBOO) | 48 | Ripepi et al. (2014) | ||||||
| Eclipsing Binaries (EA+EB+EW) | 13 | A90; A95: A02; B81; L97; L02; L04; L09; MP08; S82; S84; C04b | ||||||
| Long-Period Variables (LPV) | ~260 | Olivier et al. (2001); Smith et al. (2002); Whitelock et al. (2000, 2006) | ||||||
| Quasi-Stellar Objects (QSO) | ~70 | Cioni et al. (2013) | ||||||
| R Coronae Borealis (RCB) | 12 | Feast et al. (1997) | ||||||
| RR Lyrae, type RRab (RRab) | 44 | B92; C92; DP05; F89; F90a; J88; J92; J96; S89; S93; ST92; R12(a, b); M14; Sz14c | ||||||
| RR Lyrae, type RRc (RRc) | 8 | F90b; D05; J96; R12(a, b); M14d | ||||||
| T Tauri stars (INT) | 1 | Lorenzetti et al. (2007) | ||||||
| Wolf-Rayet stars (WR) | 6 | Van der Hucht et al. (2001); Williams et al. (1990, 2012, 2013) | ||||||
Reference.
P04: Persson et al. (2004); G13: Groenewegen (2013); MP11: Monson & Pierce (2011); Ripepi et al. (2012a,b); Moretti et al. (2014).
A90: Arevalo & Lázaro (1990); A95: Arevalo et al. (1995); A02: Arevalo et al. (2002); B81: Bailey et al. (1981); L97: Lázaro et al. (1997); L02: Lázaro et al. (2002); L04: Lázaro et al. (2004); L09: Lázaro et al. (2009); MP08: Martínez-Pais et al. (2008); S82: Sherrington et al. (1982); S84: Sherrington et al. (1984); C04: Covino et al. (2004).
B92: Barnes et al. (1992); C92: Cacciari et al. (1992); DP05: Del Principe et al. (2005); F89: Fernley et al. (1989); F90: Fernley et al. (1990a); J88: Jones et al. (1988); J92: Jones et al. (1992); J96: Jones et al. (1996); S89: Skillen et al. (1989); S93: Skillen et al. (1993); ST92: Storm et al. (1992); R12: Ripepi et al. (2012a,b); M14: Moretti et al. (2014); Sz14: Szabó et al. (2014).
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