Determining the true mass of radial-velocity exoplanets with Gaia - Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets

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Table 7

Two exoplanets, WASP-43 b and WASP-156 b, whose RV orbits are incompatible with Gaia astrometric excess noise.

Parameter	Unit	WASP-43 b	WASP-156 b
Period	(day)	0.813	3.836
m sin i	(M_J)	1.761	0.131
a sin i	(mas)	0.00047	0.000055
ε_DR1	(mas)	1.96	1.49
ε_simu,max	(mas)	1.25	1.32

Notes. The maximum astrometric excess noise that we were able to simulate for these secondary dataset sources is given as ε_simu,max.

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