The GAPS Programme with HARPS-N at TNG - XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

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Volume 602 (June 2017)

A&A, 602 (2017) A107

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Table 7

System parameters that were used, along with the orbital parameters in Table 8, to update the mass, density, and surface gravity of the 231 transiting giant planets in our sample (see Table 9).

System	M _s	R _s	T _eff	[ Fe / H ]	V sin i	P _rot	Age	i _p	R _p	System
	[M_⊙]	[R_⊙]	[K]	[dex]	[]	[day]	[Gyr]	[deg]	[R_Jup]	reference

CoRoT-1	1.220 ± 0.030	1.230 ± 0.020	6298 ± 66	0.060 ± 0.070	5.2 ± 1.0	–	1.60 ± 0.50	85.10 ± 0.50	1.715 ± 0.030	1, this work¹
CoRoT-2	0.970 ± 0.060	0.902 ± 0.018	5625 ± 120	0.0 ± 0.1	11.85 ± 0.50	4.522 ± 0.024				2, 3, 4, 5
CoRoT-3	1.370 ± 0.090	1.560 ± 0.090	6740 ± 140	− 0.020 ± 0.060	17.0 ± 1.0	–	2.20 ± 0.60	85.90 ± 0.80	1.010 ± 0.070	6
CoRoT-4			6190 ± 60	0.050 ± 0.070	6.4 ± 1.0	8.9 ± 1.1			1.190 ± 0.055	7
CoRoT-5	1.000 ± 0.020	1.186 ± 0.040	6100 ± 65	− 0.250 ± 0.060	1.0 ± 1.0	–	6.9 ± 1.4			8
CoRoT-6	1.050 ± 0.050	1.025 ± 0.026	6090 ± 50	− 0.200 ± 0.100	7.5 ± 1.0	6.40 ± 0.50		89.07 ± 0.30	1.166 ± 0.035	9, 10
CoRoT-8	0.880 ± 0.040	0.770 ± 0.020	5080 ± 80	0.300 ± 0.100	2.0 ± 1.0	–		88.400 ± 0.100	0.570 ± 0.020	11
CoRoT-9	0.960 ± 0.040	0.960 ± 0.060	5625 ± 80	− 0.010 ± 0.060		–	6.0 ± 3.0			12
CoRoT-10	0.890 ± 0.050	0.790 ± 0.050	5075 ± 75	0.260 ± 0.070	2.00 ± 0.50	–		88.55 ± 0.20	0.970 ± 0.070	13
...	...	...	...	...	...	...	...	...	...	...
Kepler-76	1.20 ± 0.20	1.320 ± 0.080	6409 ± 95	− 0.10 ± 0.20	6.5 ± 2.0	–		78.00 ± 0.20	1.250 ± 0.080	14, this work²
...	...	...	...	...	...	...	...	...	...	...

Notes. The vast majority of system parameters are taken from the literature, although estimates of ages for 37 systems with stellar evolutionary tracks are provided here for the first time (Sect. 4). In a very few cases, namely CoRoT-1, WASP-63, WASP-78, and WASP-79, we adopted our values of stellar mass and stellar/planetary radii (see Sect. 4). Full table available at the CDS. A portion is shown here for guidance regarding its form and content.

⁽¹⁾

The new system parameters M_s, R_s, R_p, and age were derived by using the Y2 evolutionary tracks and the published values of stellar atmospheric parameters, stellar density from the transit fitting, and R_p/R_s (as reported in the corresponding reference).

⁽²⁾

The system age was estimated by using the Y2 evolutionary tracks and the published values of stellar atmospheric parameters and stellar density from the transit fitting (as reported in the corresponding reference).

Reference. (1) Barge et al. (2008) and Torres et al. (2012); (2) Bouchy et al. (2008); (3) Alonso et al. (2008); (4) Gillon et al. (2010); (5) Lanza et al. (2009); (6) Deleuil et al. (2008); (7) Moutou et al. (2008); (8) Rauer et al. (2009); (9) Fridlund et al. (2010); (10) Southworth (2011); (11) Bordé et al. (2010); (12) Bonomo et al. (2017); (13) Bonomo et al. (2010); ... (14) Faigler et al. (2013); ...

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