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Table 11
Comparison between the planet and binary scenarios for candidates around M-dwarfs.
| Object | V | dp(%) |
|
|
dp |
dp (%) |
|
|
|
|
||||||||
| 19b4-10711 | 0.69 | 23.70 | 1.7020 | 1.6952 | 23.87 | 25.90 | 0.86 | 0.66 |
| 19e3-01290 | 0.66 | 24.98 | 1.0759 | 1.0715 | 25.52 | 19.95 | 0.71 | 0.52 |
| 19a2-10046 | 0.61 | 19.63 | 2.0426 | 2.0596 | 19.52 | 17.54 | 0.62 | 0.64 |
| 19a1-02980 | 0.72 | 2.17 | 1.7077 | 1.6537 | 2.70 | 1.42 | 0.71 | 0.79 |
| 19a1-07499 | 0.68 | 7.38 | 1.3803 | 1.3759 | 7.10 | 8.01 | 0.60 | 0.90 |
| 19e3-05850 | 0.00 | 7.85 | 1.1237 | 1.1203 | 7.48 | 7.42 | 0.00 | 0.16 |
| 19a1-10878 | 0.65 | 22.70 | 1.9194 | 1.7947 | 24.19 | 19.06 | 0.65 | 0.80 |
| 19a1-01358 | 0.91 | 4.67 | 1.3165 | 1.3142 | 5.28 | 3.30 | 0.66 | 0.21 |
Notes. Comparison of the eclipse shapes, eclipse depths, and values of the planet scenario and binary scenario (prime values on the right side of the table).
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