Table 5
Summary of the strongest periods found in the different periodograms.
| Star | Pmax | RV | FWHM | BIS | Hα06 | Hα16 | Phot | RV | FWHM | BIS | Hα06 | Hα16 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| NGC 368ONo. 41 | – | 1128 | – | – | – | – | – | – | – | – | – | |
| NGC 2345No. 50 | 1463 | 1007 | 957 | 1409 | 962 | 1113 | 561 | – | – | 586 | 545 | |
| NGC 3532No. 670 | 447 | 842 | 811 | – | – | 889 | 625 | 619 | – | 574 | ||
| IC4651No. 9122 | 995 | 744 | – | – | – | 985 | – | 384 | 364/393 | – | – | – |
| NGC 2423No. 3 | 407 | 697 | – | 697 | – | – | 435 | – | ||||
| NGC 4349No. 127 | 399 | 674 | 675 | – | – | – | – | – | – | – | ||
Notes. First set of columns: Maximum stellar rotational period and periods of the most significant peak(s) in each GLS periodogram that match the most significant RV period. We highlight in blue the periods that are compatible with the estimated stellar rotation period. Second set of columns: For the stars with a possible two-Keplerian fit, we list the periods of the periodogram peaks that match the period of the hypothetical second companion in the system. The periodogram peaks that lie above the 1 % FAP level are marked in boldface.
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