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Table 2
Orbital ephemerides from the Bayesian parameter estimation algorithm.
| Parameter | A36 | B17 | MT059 | MT696 | MT720 | Schulte 3 | Schulte 5 |
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|
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| HJD0 | 56 282.520 | 56 383.961 | 56 535.672 | 56 181.719 | 56 585.602 | 56 264.633 | 56 182.906 |
| Pemp (d) | 4.676040(21) | 4.021767(38) | 4.852281(39) | 1.46918869(22) | 4.3619709(98) | 4.745964(15) | 6.597989(24) |
| Ṗemp(×10-8) | 3.8 ± 1.3 | 1.1 ± 1.6 | -4.7 ± 1.7 | -0.37 ± 0.08 | 8.1 ± 2.1 | -1.5 ± 1.0 | 1.16 ± 0.03 |
| Pmodel (d) | 4.676040(19) | 4.021719(39) | 4.852265(26) | 1.46918857(24) | 4.3617773(96) | 4.745998(29) | 6.5980120(30) |
| Ṗmodel(×10-8) | 3.9 ± 1.3 | -08 ± 1.7 | -3.6 ± 1.2 | -0.46 ± 0.08 | -11.7 ± 3.2 | -0.0 ± 0.9 | 1.30 ± 0.03 |
Notes. We list the epoch of periastron (HJD0), period (P), and the rate of period change (Ṗ). The parameters P and Ṗ are calculated using empirical (emp) and PHOEBE (model) phased light curves. HJD0 is fixed in both cases.
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