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Table 5
Comparison between the planet and binary scenarios.
Object | V | dp(%) |
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dp![]() |
dp![]() |
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19b1-02162 | 0.25 | 2.05 | 1.3792 | 1.3438 | 2.54 | 1.37 | 0.25 | 0.00 |
19f3-06991 | 0.56 | 0.81 | 1.0087 | 0.9545 | 1.08 | 0.47 | 0.58 | 0.33 |
19b3-09004 | 0.31 | 3.07 | 4.3247 | 4.2817 | 3.44 | 2.87 | 0.54 | 0.01 |
19g1-11212 | 0.37 | 1.49 | 1.4751 | 1.4301 | 2.29 | 1.34 | 0.45 | 0.81 |
19c4-02952 | 0.57 | 4.13 | 3.3622 | 3.3617 | 3.73 | 3.86 | 0.00 | 0.53 |
19h1-00325 | 0.43 | 3.11 | 4.0514 | 4.0172 | 2.92 | 3.05 | 0.16 | 0.38 |
19b3-05398 | 0.29 | 2.66 | 0.9802 | 0.9739 | 2.91 | 2.55 | 0.48 | 0.36 |
19e1-05755 | 0.29 | 1.76 | 1.7486 | 1.7211 | 2.54 | 1.66 | 0.80 | 0.54 |
19b4-04138 | 0.64 | 2.53 | 1.7270 | 1.7041 | 2.51 | 2.36 | 0.66 | 0.62 |
19b2-01819 | 0.45 | 2.80 | 2.7123 | 2.6819 | 2.74 | 3.07 | 0.61 | 0.65 |
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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