2016AJ....151..138R

We report the discovery of KELT-14b and KELT-15b, two hot Jupiters from the KELT-South survey. KELT-14b, an independent discovery of the recently announced WASP-122b, is an inflated Jupiter mass planet that orbits a ∼{5.0}_{-0.7}^{+0.3} Gyr, V=11.0, G2 star that is near the main sequence turnoff. The host star, KELT-14 (TYC 7638-981-1), has an inferred mass {M}_{*} = {1.18}_{-0.07}^{+0.05} M_☉ and radius {R}_{*} = 1.37±-0.08 R_☉, and has {T}_{eff} = {5802}_{-92}^{+95} K, log{g}_{*} = {4.23}_{-0.04}^{+0.05} and [Fe/
H] =0.33±-0.09. The planet orbits with a period of 1.7100588±0.0000025 days (T₀=2457091.02863±0.00047) and has a radius R_p= {1.52}_{-0.11}^{+0.12} R_J and mass M_p=1.196±0.072 M_J, and the eccentricity is consistent with zero. KELT-15b is another inflated Jupiter mass planet that orbits a ∼ {4.6}_{-0.4}^{+0.5} Gyr, V=11.2, G0 star (TYC 8146-86-1) that is near the "blue hook" stage of evolution prior to the Hertzsprung gap, and has an inferred mass {M}_{*} = {1.181}_{-0.050}^{+0.051} M_☉ and radius {R}_{*} = {1.48}_{-0.04}^{+0.09} R_☉, and {T}_{eff} = {6003}_{-52}^{+56} K, log{g}_{*} = {4.17}_{-0.04}^{+0.02} and [Fe/
H] =0.05±0.03. The planet orbits on a period of 3.329441±0.000016 days (T₀=2457029.1663±0.0073) and has a radius R_p= {1.443}_{-0.057}^{+0.11} R_J and mass M_p= {0.91}_{-0.22}^{+0.21} M_J and an eccentricity consistent with zero. KELT-14b has the second largest expected emission signal in the K-band for known transiting planets brighter than K