Table 1
The studied sample of RVb stars.
| Name | Tobs | Nobs | Ppul | Pmod | Source |
| (d) | (d) | (d) | |||
|
|
|||||
| IW Car | 18 120 | 4685 | 71.98 | 1449 | AAVSO |
| 3300 | 2179 | 72.2 | 1470 | ASAS | |
| SX Cen | 22 409 | 1320 | 32.88 | 602 | AAVSO |
| 3296 | 1153 | 33.01 | 610 | ASAS | |
| DF Cyg | 17 074 | 5924 | 49.82 | 780 | AAVSO |
| 1470 | 66 533 | 49.84 | 786 | Kepler | |
| SU Gem | 14 783 | 2228 | 49.92 | 682 | AAVSO |
| U Mon | 46 283 | 48 019 | 91.48 | 2451 | AAVSO |
| AR Pup | 14 998 | 1450 | 76.66 | 1194 | AAVSO |
| 3299 | 1086 | 76.34 | 1178 | ASAS | |
| AI Sco | 19 538 | 1408 | 71.64 | 977 | AAVSO |
| RV Tau | 40 020 | 14 976 | 78.48 | 1210 | AAVSO |
| BLG-T2CEP-177 | 2836 | 742 | 92.44 | 2970 | OGLE |
| BLG-T2CEP-215 | 2829 | 814 | 55.74 | 958 | OGLE |
| BLG-T2CEP-345 | 2830 | 1344 | 73.64 | 1100 | OGLE |
| BLG-T2CEP-350 | 2776 | 1026 | 87.20 | 722 | OGLE |
| BLG-T2CEP-352 | 4404 | 978 | 103.78 | 543 | OGLE |
| BLG-T2CEP-354 | 3232 | 533 | 66.46 | 951 | OGLE |
| LMC-T2CEP-200 | 4494 | 917 | 69.86 | 850 | OGLE |
Notes. Tobs and Nobs are the time-span and the total number of observations. Ppul and Pmod refer to the periods of pulsation and RVb-type modulation, respectively, as measured from the analysed data. The OGLE variable names were shortened by omitting “OGLE-” in front of the shown identifiers.
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