Table 3
Fourteen planetary systems with measured λ and/or ψ with a stellar Teff ≤ 5000 K.
System | Teff | λ | ψ | Reference |
---|---|---|---|---|
(K) | (°) | (°) | ||
GJ 0436 | 3416 ± 54 | ![]() |
![]() |
(Bourrier et al. 2018) |
HAT-P-11 | 4780 ± 50 | ![]() |
(Winn et al. 2010b) | |
HAT-P-11 | 4780 ± 50 | ![]() |
(Hirano et al. 2010) | |
HAT-P-11 | 4780 ± 50 | ![]() |
![]() |
Solution 1 (Sanchis-Ojeda & Winn 2011) |
HAT-P-11 | 4780 ± 50 | ![]() |
![]() |
Solution 2 (Sanchis-Ojeda & Winn 2011) |
HAT-P-11 | 106.6 ± 8.3 | |||
HAT-P-12 | 4665 ± 45 | ![]() |
(Mancini et al. 2018) | |
HAT-P-18 | 4870 ± 50 | 132 ± 15 | (Esposito et al. 2014) | |
HAT-P-20 | 4595 ± 45 | -8.0 ± 6.9 | ![]() |
(Esposito et al. 2017) |
Qatar-1 | 4910 ± 100 | -8.4 ± 7.1 | (Covino et al. 2013) | |
Qatar-2 | 4645 ± 50 | 4.3 ± 4.5 | (Mancini et al. 2014) | |
Qatar-2 | 4645 ± 50 | 0.0 ± 8.0 | (Močnik et al. 2017) | |
Qatar-2 | 4645 ± 50 | 0.0 ± 10.0 | (Dai et al. 2017) | |
Qatar-2 | 4645 ± 50 | 15 ± 20 | ![]() |
(Esposito et al. 2017) |
Qatar-2 | 3.2 ± 3.6 | |||
WASP-11 | 4900 ± 65 | 7 ± 5 | (Mancini et al. 2015) | |
WASP-43 | 4520 ± 120 | 3.5 ± 6.8 | ![]() |
(Esposito et al. 2017) |
WASP-52 | 5000 ± 100 | ![]() |
(Hébrard et al. 2013) | |
WASP-52 | 5000 ± 100 | 3.8 ± 8.4 | 20 ± 50 | (Mancini et al. 2017) |
WASP-52 | 9.7 ± 7.1 | |||
WASP-53 | 4950 ± 60 | -1.0 ± 12 | (Triaud et al. 2017) | |
WASP-69 | 4700 ± 50 | ![]() |
(Casasayas-Barris et al. 2017) | |
WASP-80 | 4145 ± 100 | 0 ± 20 | (Triaud et al. 2013) | |
WASP-80 | 4145 ± 100 | − 14 ± 14 | (Triaud et al. 2015) | |
WASP-80 | -9.4 ± 11.5 | |||
WASP-107(a) | 4430 ± 120 | 90 ± 50 | (Dai et al. 2017) |
Notes. All multiple measurements for the same object are included together with the associated weighted mean. The values in bold were used to determine the weighted mean of λ from the 13 planetary systems with a measured λ. Obtained from the 2019/12/30 version of the TEPCat catalogue (Southworth 2011). (a) Dai et al. (2017) only gives a measurement of ψ for WASP-107. Therefore, WASP-107 was not used in calculating the weighted mean of λ.
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