2017MNRAS.468..835B

We report the discovery of three moderately high-mass transiting hot Jupiters from the HATSouth survey: HATS-22b, HATS-23b and HATS-24b. These planets add to the number of known planets in the ∼2M_J regime. HATS-22b is a 2.74 ± 0.11 M_J mass and 0.953_–0.029^+0.048 R_ J_ radius planet orbiting a V = 13.455 ± 0.040 sub-solar mass (M_* = 0.759 ± 0.019 M_☉; R_* = 0.759 ± 0.019 R_☉) K-dwarf host star on an eccentric (e = 0.079 ± 0.026) orbit. This planet's high planet-to-stellar mass ratio is further evidence that migration mechanisms for hot Jupiters may rely on exciting orbital eccentricities that bring the planets closer to their parent stars followed by tidal circularization. HATS-23b is a 1.478 ± 0.080 M_J mass and 1.69 ± 0.24 R_J radius planet on a grazing orbit around a V = 13.901 ± 0.010 G-dwarf with properties very similar to those of the Sun (M_* = 1.115 ± 0.054; R_* = 1.145 ± 0.070). HATS-24b orbits a moderately bright V = 12.830 ± 0.010 F-dwarf star (M_* = 1.218 ± 0.036 M_☉; R_*=_1.194-0.041+0.066^ R_☉). This planet has a mass of 2.39_–0.12^+0.21 M_ J_ and an inflated radius of 1.516_–0.065^+0.085 R_ J_.