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Table 1
Rate of eclipse identification by the two models on the set of 2861 phase-folded Kepler and Gaia-sampled light curves.
| Primary | Secondary | |
| Model (Kepler data set) | eclipse [%] | eclipse [%] |
|
|
||
| Polyfit and two-Gaussian | 95.3 | 66.8 |
| None | 0.0 | 14.1 |
| Only polyfits | 4.7 | 3.7 |
| Only two-Gaussian | 0.0 | 15.4 |
|
|
||
| Data set (two-Gaussian model) | ||
|
|
||
| Kepler and Gaia-sampled | 63.8 | 50.0 |
| None | 4.7 | 16.5 |
| Only Kepler | 31.4 | 32.2 |
| Only Gaia-sampled | 0.10 | 1.3 |
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