Abstract
We report the discovery of HATS-15 b and HATS-16 b, two massive transiting extrasolar planets orbiting evolved (∼10 Gyr) main-sequence stars. The planet HATS-15 b, which is hosted by a G9 V star ( mag), is a hot Jupiter with mass of and radius of , and it completes its orbit in about 1.7 days. HATS-16 b is a very massive hot Jupiter with mass of and radius of it orbits around its G3 V parent star ( mag) in ∼2.7 days. HATS-16 is slightly active and shows a periodic photometric modulation, implying a rotational period of 12 days, which is unexpectedly short given its isochronal age. This fast rotation might be the result of the tidal interaction between the star and its planet.
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More From: Publications of the Astronomical Society of the Pacific
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