Table 3.
Parameters for four stars with a detection of additional signals.
| Name | P1O [d] | PX [d] | PS/PL |
|---|---|---|---|
| BG CruF | 3.34260(9) | 2.03330(9) | 0.60830 |
| BG CruC | 3.34260(1) | 2.0340(2) | 0.60838 |
| V0391 NorF | 4.3727(1) | 2.7817(2) | 0.63616 |
| V0391 NorB | 4.3729(4) | 2.7817(2) | 0.63612 |
| QZ NorR | 3.786803(8) | 4.847(2) | 0.78127 (0.63998) |
| QZ NorF | 3.78659(7) | 4.847(2) | 0.78117 (0.64007) |
| QZ NorB | 3.7872(1) | 4.846(1) | 0.78158 (0.63973) |
| V0411 LacF | 2.9088(1) | 4.2370(1) | 0.68652 |
| V0411 LacB | 2.90847(3) | 4.228(2) | 0.68792 |
Notes. The consecutive columns provide the name of the star, the first-overtone period, the period of the additional signal, and their shorter-to-longer period ratio. There are multiple rows for stars for which a detection was made in different datasets: RV (R), FWHM (F), BIS (B), and contrast (C). For QZ Nor, we include in parentheses the period ratio that would be formed by the harmonic of the detected additional signal (see text for details).
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