SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter

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Volume 564 (April 2014)

A&A, 564 (2014) A56

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Table 5

Planetary systems with phase curve and/or secondary detected.

System	T _eff	a	T _eq	M _p	R _p	P


Kepler-5^1,2,3	6297 ± 60	0.05064 ± 0.0018	1752 ± 17	2.112	1.431	3.5484
Kepler-6^4,2,3	5647 ± 44	0.04561 ± 0.0006	1451 ± 16	0.668	1.323	3.2347
Kepler-7^5,3	5933 ± 44	0.06246 ± 0.00046	1586 ± 13	1.443	1.614	4.8854
Kepler-8^6,2,3	6210 ± 150	0.04833 ± 0.002	1638 ± 40	0.583	1.419	3.5225
Kepler-12^7,3	5947 ± 100	0.05563 ± 0.007	1477 ± 26	0.432	1.695	4.438
Kepler-17^8,9,3	5781 ± 85	0.0268 ± 0.0005	1655 ± 40	2.477	1.330	1.4857
Kepler-41^10,11,3	5620 ± 140	0.0303 ± 0.0009	1567 ± 41	0.540	1.240	1.8555
KOI-13^12,13,2	8500 ± 400	0.0514 ± 0.0020	2885 ± 140	8.500	2.042	3.5225
HAT-P-7^14,2,3	6350 ± 80	0.0355 ± 0.0044	2139 ± 27	1.779	1.363	2.204
TRES-2^15,2,3	5850 ± 50	0.0367± 0.0013	1444 ± 13	1.193	1.224	2.470
CoRoT-1¹⁶	5950 ± 150	0.0254 ± 0.0004	1896 ± 52	1.037	1.490	1.5089
CoRoT-2^17,18	5625 ± 120	0.0281 ± 0.0004	1536 ± 35	3.273	1.466	1.742

Notes. In some cases, asymmetric error bars have been symmetrized.

Reference.

⁽¹⁾

Koch et al. (2010);

⁽²⁾

Esteves et al. (2013);

⁽³⁾

Heng & Demory (2013);

⁽⁴⁾

Dunham et al. (2010);

⁽⁵⁾

Demory et al. (2011);

⁽⁶⁾

Jenkins et al. (2010);

⁽⁷⁾

Fortney et al. (2011);

⁽⁸⁾

Désert et al. (2011);

⁽⁹⁾

Bonomo et al. (2012);

⁽¹⁰⁾

Santerne et al. (2011);

⁽¹¹⁾

Bonomo et al. (2013);

⁽¹²⁾

Szabó et al. (2011);

⁽¹³⁾

Mazeh et al. (2012);

⁽¹⁴⁾

Christiansen et al. (2010);

⁽¹⁵⁾

Barclay et al. (2012);

⁽¹⁶⁾

Alonso et al. (2009a);

⁽¹⁷⁾

Snellen et al. (2009);

⁽¹⁸⁾

Alonso et al. (2009b).

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