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Table 3
Pearson and Stockman correlation coefficients of the computed pEW of the emission lines considered in this work vs. the pEW of Hα.
| All, N = 386 | 6417d, N = 55 | 6418d, N = 23 | ||||
|---|---|---|---|---|---|---|
| Hα vs. line | kp | ks | kp | ks | kp | ks |
| CaII (K) | 0.8045 | 0.7229 | 0.9531 | 0.7832 | 0.8042 | 0.7955 |
| CaII (H) | 0.8897 | 0.7847 | 0.9753 | 0.8188 | 0.8068 | 0.8098 |
| He5876 | 0.9288 | 0.8389 | 0.9377 | 0.7286 | 0.6407 | 0.6055 |
| He4026 | 0.5265 | 0.4420 | ||||
| Hɛ | 0.9068 | 0.7506 | 0.9210 | 0.8353 | 0.5907 | 0.6118 |
| NaI(D2) | 0.9397 | 0.8824 | 0.9456 | 0.7877 | 0.9673 | 0.9555 |
| NaI(D1) | 0.9496 | 0.8832 | 0.9489 | 0.8108 | 0.9628 | 0.9617 |
Notes. Dates between BJD = 6417 and 6429 were not accounted for He4026 line (see Sect. 4.2).
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