KELT-6 13 03 55.6468 +30 38 24.2797 222 KELT-6 TYC 2532-556-1 BD+31 2447 2MASS J13035564+3038241 Gaia DR2 1464700950221781504 1.126 1.529 6272 10.337 9.745 9.137 10.81 9.30 9.08 -0.27 F8 4.90 KELT-6 b TYC 2532-556-1 b BD+31 2447 b Gaia DR2 1464700950221781504 b Confirmed planets 0.442 1.18 7.845582 0.080 0.029 88.81 2457124.50954 308 -36 KELT-6b is a Saturn-mass planet transiting a metal-poor host star. The planet candidate was originally discovered by the KELT-North survey. Follow up observations confirmed the planetary nature of the candidate using a combination of photometry, high-resolution imaging, high resolution spectroscopy and radial velocity measurements. transit 15/08/27 2013 1 KELT-6 c TYC 2532-556-1 c BD+31 2447 c Gaia DR2 1464700950221781504 c Confirmed planets 1276 0.21 268.7 2457432 3.71 2.39 KELT-6c is a long-period giant planet, one of only a small number known where there is an inner transiting planet with a measured Rossiter-McLaughlin effect. Its presence was suspected based on a trend in the radial velocity data for the system and was finally confirmed in 2015 with data from the HARPS-N spectrograph. RV 15/08/27 2015 0 Coma Berenices