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Table 4

Variability parameters and source classification.

ID (a) max(∆S /σ) (b) α¯±σα¯$\bar \alpha \pm \sigma \bar \alpha $ (c) Ξ (d) stype (e) Source classification (f)
qF257 143.3 ± 4.9 0.24 ± 0.03 14.5 ± 11.8 B1-2Ia+ pCWB
qF241 13.7 ± 3.9 0.68 ± 0.02 11.5 ± 5.8 WN11h Th.
qF362 35.9 ± 2.9 1 .44 ± 0.06 27.9 ± 9.1 LBV Th.
qF240 6.8 ± 3.7 0.87 ± 0.07 10.0 ± 8.4 WN10h Th.
qF320 7.7 ± 3.5 0.84 ± 0.04 27.9 ± 9.3 WN9h sCWB
Muno7679 6.9 ± 3.4 −0.32 ± 0.07 8.5 ± 5.0 pCWB
Dong66 19.8 ± 3.6 0.12 ± 0.08 20.1 ± 5.3 O7-B0 I pCWB
qF211 7.0 ± 3.7 0.34 ± 0.14 6.7 ± 3.5 WC9d(+OB) sCWB
qF256 14.3 ± 4.2 0.62 ± 0.06 21.6 ± 12.6 WN8-9ha sCWB
qF23l 6.0 ± 3.2 0.83 ± 0.16 7.2 ± 2.9 WC9d(+OB) sCWB
qF270S 6.7 ± 3.1 0.43 ± 0.21 9.1 ± 4.1 B1-2Ia+/WNLh a
qF235S 1.9 ± 1.9 0.47 ± 0.20 10.8 ± 4.8 WC8(d?+OB?) a
qF307A 5.6 ± 3.5 0.28 ± 0.17 7.2 ± 7.2 B1-2(Ia+) a
qF344 9.5 ± 3.4 −0.21 ± 0.08 23.5 ± 7.8 O7-8Ia pCWB
qF235N 6.2 ± 4.0 0.57 ± 0.20 14.8 ± 4.8 WC8(d?+OB?) a
qF353E 6.3 ± 3.5 0.72 ± 0.48 2.4 ± 0.9 WN6 a
qF381 5.2 ± 2.3 0.33 ± 0.40 2.0 ± 1.4 B0-1Ia+/WNLh a
qCG1 2.7 ± 3.1 −0.82 ± 0.24 9.1 ± 3.7 pCWB
qF278 4.4 ± 3.4 −0.23 ± 0.58 B0-1(Ia+) a?
qF309 6.3 ± 4.4 0.19 ± 0.41 0.3 ± 0.3 WC8-9(d?+OB?) a
LHO100 7.9 ± 3.3 0.00 ± 0.66 B2-3Ia+ a
qF274 1.8 ± 1.8 0.43 ± 0.19 6.2 ± 3.0 WN8-9ha a?
Hos332 7.2 ± 3.3 −0.84 ± 0.31 0.7 ± 0.6 pCWB
LHO076 3.5 ± 2.6 0.47 ± 0.10 WC9d(+OB) Th.
WR102ca 6.6 ± 4.5 1.79 ± 0.14 WC9d(+OB) Th.
LHO090 3.9 ± 3.1 −0.93 ± 0.08 12.4 ± 7.4 O9-B0Ia pCWB
qF258 5.1 ± 2.5 1.81 ± 0.29 WC9d(+OB) Th.
qF134 44.6 ± 3.3 1.78 ± 0.17 6.4 ± 2.6 LBV Th.

Notes. (a) Boldface in ID indicates X-ray counterparts from Muno et al. (2009).(b) Maximum value obtained from ∆S/σ in any band.(c) Spectral index’s weighted mean.(d) Value obtained from Eq. (3). Uncertainties were derived using standard error propagation. (e) Spectral type from Clark et al. (2018b) or Dong et al. (2011).(f) Source classification: pCWB = primary CWB candidate, sCWB = secondary CWB candidate, Th. = thermal source, a = ambiguous source.

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