HAT-P-12b: A Low-Density Sub-Saturn Mass Planet Transiting a Metal-Poor K Dwarf
J. D. Hartman (1), G. \'A. Bakos (1,2), G. Torres (1), G\'eza Kov\'acs, (3), R. W. Noyes (1), A. P\'al (1,3,4), D. W. Latham (1), B. Sip\"ocz (1,4),, D. A. Fischer (5), J. A. Johnson (6), G. W. Marcy (7), R. P. Butler (8), A., W. Howard (7), G. A. Esquerdo (1)

TL;DR
HAT-P-12b is a low-density, sub-Saturn mass exoplanet orbiting a metal-poor K dwarf, notable for being the least massive H/He dominated gas giant discovered to date, with detailed characterization and ruling out false positives.
Contribution
This study reports the discovery and detailed characterization of HAT-P-12b, the least massive H/He gas giant known, including analysis of its orbit, mass, radius, and composition.
Findings
HAT-P-12b has a mass of 0.211 MJup and radius of 0.959 RJup.
The planet's density is approximately 0.295 g/cm^3.
It is consistent with a 1-4.5 Gyr, mildly irradiated, H/He dominated planet with a small core.
Abstract
We report on the discovery of HAT-P-12b, a transiting extrasolar planet orbiting the moderately bright V=12.8 K4 dwarf GSC 03033-00706, with a period P = 3.2130598 +- 0.0000021 d, transit epoch Tc = 2454419.19556 +- 0.00020 (BJD) and transit duration 0.0974 +- 0.0006 d. The host star has a mass of 0.73 +- 0.02 Msun, radius of 0.70 +- ^0.02_0.01 Rsun, effective temperature 4650 +- 60 K and metallicity [Fe/H] = -0.29 +- 0.05. We find a slight correlation between the observed spectral line bisector spans and the radial velocity, so we consider, and rule out, various blend configurations including a blend with a background eclipsing binary, and hierarchical triple systems where the eclipsing body is a star or a planet. We conclude that a model consisting of a single star with a transiting planet best fits the observations, and show that a likely explanation for the apparent correlation is…
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