HATS-60b─HATS-69b: 10 Transiting Planets from HATSouth

Hartman, J. D. and Bakos, Gáspár and Bayliss, D. and Bento, J. and Bhatti, W. (2019) HATS-60b─HATS-69b: 10 Transiting Planets from HATSouth. ASTRONOMICAL JOURNAL, 157 (2). ISSN 0004-6256

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Abstract

We report the discovery of 10 transiting extrasolar planets by the HATSouth survey. The planets range in mass from the super-Neptune HATS- 62b, with {M}p< 0.179 {M}{{J}}, to the super- Jupiter HATS-66b, with {M}p=5.33 {M}{{J}}, and in size from the Saturn HATS-69b, with {R}p=0.94 {R}{{J}}, to the inflated Jupiter HATS-67b, with {R}p=1.69 {R}{{J}}. The planets have orbital periods between 1.6092 days (HATS-67b) and 7.8180 days (HATS-61b). The hosts are dwarf stars with masses ranging from 0.89 {M}ȯ (HATS-69) to 1.56 {M}ȯ (HATS-64) and have apparent magnitudes between V=12.276+/- 0.020 mag (HATS-68) and V=14.095+/- 0.030 mag (HATS-66). The super-Neptune HATS-62b is the least massive planet discovered to date with a radius larger than Jupiter. Based largely on the Gaia DR2 distances and broadband photometry, we identify three systems (HATS-62, HATS-64, and HATS-65) as having possible unresolved binary star companions. We discuss in detail our methods for incorporating the Gaia DR2 observations into our modeling of the system parameters and into our blend analysis procedures. The HATSouth network is operated by a collaboration consisting of Princeton University (PU), the Max Planck Institute für Astronomie (MPIA), the Australian National University (ANU), and the Pontificia Universidad Católica de Chile (PUC). The station at Las Campanas Observatory (LCO) of the Carnegie Institute is operated by PU in conjunction with PUC, the station at the High Energy Spectroscopic Survey (H.E.S.S.) site is operated in conjunction with MPIA, and the station at Siding Spring Observatory (SSO) is operated jointly with ANU. Based in part on observations made with the MPG 2.2 m Telescope at the ESO Observatory in La Silla. Based on observations collected at the European Southern Observatory under ESO programs 094.C-0428(A), 095.C-0367(A), 097.C-0571(A), 098.C-0292(A), 099.C-0374(A), 0100.C-0406(A), and 0100.C-0406(B). This paper includes data gathered with the 6.5 m Magellan Telescopes at Las Campanas Observatory, Chile. Based in part on observations made with the Anglo- Australian Telescope operated by the Australian Astronomical Observatory.

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