Table 3.
Orbital period measurements for the different datasets used.
| Observer | Filter | PGLS | PPDM |  |
|---|---|---|---|---|
| Lorenzi1980 | V | 11.084(003) | 11.100(050) | 11.090(030) |
| AAVSO | V | 11.087(001) | – | 11.087(001) |
| Hipparcos | Hp | 11.770(010) | – | 11.770(010) |
| NSVS | V | 11.800(200) | – | 11.800(200) |
| ASAS-3 | V | 11.110(004) | 11.110(010) | 11.110(005) |
| Bochun | i | 11.110(020) | – | 11.110(020) |
| KWS | V | 11.114(002) | 11.112(009) | 11.113(005) |
| APASS | B | 11.114(009) | 11.110(040) | 11.110(020) |
| V | 11.103(009) | 11.110(040) | 11.107(020) | |
| g | 11.100(020) | 11.120(050) | 11.110(030) | |
| r | 11.090(010) | 11.110(050) | 11.100(030) | |
| i | 11.100(010) | 11.130(050) | 11.115(025) | |
| z | 10.080(090) | – | 10.080(090) | |
| Z | 11.120(030) | 11.120(050) | 11.120(030) | |
| KWS | Ic | 11.114(004) | 11.112(009) | 11.113(005) |
| ASAS-SN | V | 11.110(010) | 11.110(030) | 11.110(020) |
Notes. The values obtained by each method and their mean value are provided with their respective uncertainties, expressed as the last significant digit in parentheses. In the case that the dataset contains fewer than 100 points, the PDM method could not be implemented (see main text for details).
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