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Table 8

Derived eccentricities, RV semi-amplitudes, and trends for all the transiting giant planets considered in this study.

Planet Flag e ω ecosω esinω K Jitter
[ deg ] [ m s-1 ] [ m s-1 day-1 ] [ m s-1 ]
CoRoT-1b C <0.036 (<0.16) – 190 ± 15 <9.1
CoRoT-2b C <0.024 (<0.069) – − 0.00304 ± 0.00055 –
CoRoT-3b C <0.016 (<0.034) – 2173 ± 25 – <26.0
CoRoT-4b U <0.14 (<0.31) – – <10.5
CoRoT-5b U <0.087 (<0.19) – – <2.7
CoRoT-6b U <0.18 (<0.37) – – <15.8
CoRoT-8b U <0.19 (<0.47) – – <2.9
CoRoT-9b E 0.104 ± 0.031 0.066 ± 0.060 39.0 ± 2.4 – <3.4
CoRoT-10b E 0.524 ± 0.018 − 0.4144 ± 0.0067 – <10.7
... ... ... ... ... ... ... ... ...
HAT-P-2b E − 0.0616 ± 0.0078 CURV
... ... ... ... ... ... ... ... ...
HAT-P-17b E 0.3417 ± 0.0036 200.5 ± 1.3 − 0.3194 ± 0.0033 59.09 ± 0.65 PLC 1.4 ± 0.5
... ... ... ... ... ... ... ... ...

Notes. Both the 1σ and 2σ upper limits are given for eccentricities consistent with zero. The flag letters “C”, “E”, and “U” stand for circular, eccentric, and unconstrained orbits (the last concern either eccentricities compatible with zero but with uncertainties σe> 0.05 or slightly eccentric orbits without strong enough evidence from Bayesian model comparison; see text for more details). “CURV” or “PLC” in place of the acceleration term indicates the presence of curvature regardless of its origin (distant companion, stellar activity, possible instrumental drift) or the signal of a long-period planetary companion in the RVs. Full table available at the CDS. A portion is shown here for guidance regarding its form and content.

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