Table A.6
Maximum mass of possible trojan bodies for the six tested models assuming their presence.
|
2σ upper mass limit (M⊕) | ||||
|
|
|||||
| System | α | (M⊕) | L 4 | L 5 | α / σ α |
|
|
|||||
| corot-1b |
|
|
< −71.0 | < 50.2 | 0.4 |
| corot-2b |
|
|
< −167.4 | < 126.3 | 0.4 |
| corot-15b |
|
|
< −1352.3 | < 1763.4 | 0.3 |
| corot-18b |
|
|
< −82.0 | < 167.3 | 0.9 |
| epic211089792b |
|
|
< −93.5 | < 19.5 | 1.4 |
| gj3470b |
|
|
< −15.6 | < −1.3 | 2.5 |
| hat-p-12b |
|
|
< −39.4 | < 7.2 | 1.4 |
| hat-p-20b |
|
|
< −72.4 | < 72.3 | 0.0 |
| hat-p-23b |
|
|
< −237.7 | < 55.6 | 1.3 |
| hat-p-36b |
|
|
< −150.5 | < 530.4 | 1.1 |
| hat-p-54b |
|
|
< −258.0 | < 268.2 | 0.2 |
| hats-2b |
|
|
< −427.7 | < 416.8 | 0.1 |
| hats-9b |
|
|
< −287.4 | < 221.6 | 0.6 |
| k2-30b |
|
|
< −163.8 | < 141.5 | 0.1 |
| kepler-17b |
|
|
< −103.5 | < 160.2 | 0.4 |
| ogle-tr-113b |
|
|
< −362.7 | < 238.4 | 0.5 |
| ogle-tr-56b |
|
|
< −376.3 | < 130.1 | 0.8 |
| qatar-1b |
|
|
< −67.6 | < 79.0 | 0.1 |
| qatar-2b |
|
|
< −92.5 | < 46.6 | 0.7 |
| tres-3b |
|
|
< −105.6 | < 14.1 | 1.8 |
| tres-5b |
|
|
< −603.0 | < 576.2 | 0.1 |
| wasp-103b |
|
|
< −399.1 | < 277.3 | 0.4 |
| wasp-104b |
|
|
< −67.8 | < 76.7 | 0.1 |
| wasp-12b |
|
|
< −23.2 | < 33.6 | 0.5 |
| wasp-135b |
|
|
< −87.7 | < 87.8 | 0.0 |
| wasp-13b |
|
|
< −170.2 | < 158.5 | 0.4 |
| wasp-18b |
|
|
< −79.6 | < 59.7 | 0.3 |
| wasp-19b |
|
|
< −14.2 | < 43.1 | 1.0 |
| wasp-23b |
|
|
< −33.6 | < 34.6 | 0.0 |
| wasp-2b |
|
|
< −15.3 | < 14.6 | 0.5 |
| wasp-35b |
|
|
< −136.6 | < 159.9 | 0.4 |
| wasp-36b |
|
|
< 5.4 | < 145.8 | 2.2 |
| wasp-42b |
|
|
< −18.4 | < 23.7 | 0.3 |
| wasp-43b |
|
|
< −43.3 | < 39.9 | 0.0 |
| wasp-46b |
|
|
< −101.2 | < 77.9 | 0.2 |
| wasp-49b |
|
|
< −62.7 | < 49.9 | 0.2 |
| wasp-4b |
|
|
< −28.7 | < 7.2 | 1.1 |
| wasp-50b |
|
|
< −131.8 | < 128.1 | 0.2 |
| wasp-52b |
|
|
< −34.5 | < 41.0 | 0.1 |
| wasp-5b |
|
|
< −13.4 | < 17.9 | 0.4 |
| wasp-65b |
|
|
< −93.3 | < 84.2 | 0.2 |
| wasp-68b |
|
|
< −30.1 | < 60.3 | 0.6 |
| wasp-77ab |
|
|
< −24.4 | < 92.9 | 1.2 |
| wasp-80b |
|
|
< −28.5 | < 44.7 | 0.5 |
| wasp-98b |
|
|
< −241.2 | < 279.0 | 0.3 |
| wts-2b |
|
|
< −371.2 | < 399.4 | 0.3 |
Notes. We present the 99.7% confidence intervals of the mass computed from random samplings of the radial velocity semi-amplitude K2, the inclination i, the eccentricity e (when applicable), and the stellar mass obtained from the literature. The values listed in this table are shown in Fig. 3. (†) Estimation of the trojan mass based on α and assuming small eccentricity, mt ≪ mp, and trojan location around one the two stable Lagrangian points. Negative values correspond to L4 and positive values correspond to L5.
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.