Table A.1
Retrieved or presumed stellar parameters of the contamination stars.
| Target | Status(a) | Δmag(b) | Teff (K) | M (M⊙)(c) | R (R⊙)(c) | log g (cgs) | [M/H] | Spectral type | Comment |
|---|---|---|---|---|---|---|---|---|---|
| HAT-P-57B | C [1] | 3.85 ± 0.04 |  |
 |
 |
 |
 |
K8 – M3 | Retrieved |
| HAT-P-57C | C [1] | 3.85 ± 0.04 |  |
 |
 |
 |
 |
B8 –A6 | Retrieved |
| WASP-36 | A [2] | 5.32 ± 0.07 |  |
 |
 |
 |
 |
M3 – M5 | Retrieved |
| TrES-4 | C [3] | 4.56 ± 0.17 | 𝒰(3560, 5100) | - | - | 𝒰(4.56, 4.78) | 𝒰(−1.0,1.0) | K2 – M2 [3] | Presumed |
| WASP-2 | C [4] | 3.72 ± 0.15 | N(3523, 24) [4] | - | - | 𝒰(4.56, 4.89) | 𝒰(−1.0,1.0) | K2 – M3 [3] | Presumed |
| WASP-49 | A [5, 6] | 4.40 ± 0.39 | 𝒰(2380, 5270) | - | - | 𝒰(4.56, 5.32) | 𝒰(−1.0,1.0) | K0 – M9 | Presumed |
Notes. (a)Status of the contamination star: Ambiguous (A), Background (B), or Companion (C). (b)The difference of magnitudes between the contamination star(s) and the target star converted from the estimated flux ratio in the broadband (525 – 925 nm). In the case of HAT-P-57, Δmag consists of the two binary components.(c)The masses and radii were inferred from the PHOENIX model grids after the retrievals, which were not free parameters.
References. [1] Hartman et al. (2015) [2] Smith et al. (2012) [3] Wöllert et al. (2015) [4] Bohn et al. (2020) [5] Lendl et al. (2016) [6] Evans et al. (2016).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.