Table 2
Highest GLS peak (Phigh) and alternative GLS peak consistent with a common rotation period (Prot) (a).
| Band | Instrument | Phigh [d] | Prot [d] | |
|---|---|---|---|---|
| Single instruments | ||||
| V | ASH2 | 75.96 ± 0.27 | 68.29 ± 0.25 (b) | |
| V | SNO | 39.29 ± 1.03 | 72.32 ± 4.95 (b) | |
| V | ASAS | 3.752 ± 0.001 | 67.38 ± 0.16 (c) | |
| V | ASAS-SN | 68.49 ± 0.21 | 68.49 ± 0.21 | |
| R | ASH2 | 75.85 ± 0.33 | 68.67 ± 0.31 (d) | |
| R | SNO | 78.21 ± 1.96 | 78.21 ± 1.96 | |
| I | MEarth T 11 | 78.21 ± 7.03 | 78.21 ± 7.03 | |
| I | MEarth T 12 | 70.12 ± 7.72 | 70.12 ± 7.72 | |
| Combined instruments | ||||
| V | All | 68.40 ± 0.05 | 68.40 ± 0.05 | |
| R+I | SNO+MEarth T 11 | 41.63 ± 0.85 | 69.31 ± 2.52 (a) | |
| R+I | All | 68.46 ± 1.00 | 68.46 ± 1.00 | |
Notes. (a) We show only peaks with P > 1.2 days and FAP below 10−3. We also show the formal 1σ uncertainties provided by the GLS analysis. (b)Second highest peak of GLS. (c)Highest peak after fitting a sinusoidal for Phigh. (d) Third highest peak of GLS. Error bars denote the 68% posterior credibility intervals.
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