paper

HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs

arXiv:2002.05776 · doi:10.3847/1538-3881/ab7821

Abstract

We report the discovery of four transiting giant planets around K dwarfs. The planets HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b have masses of , , and , respectively, and radii of , , , and , respectively. The planets orbit close to their host stars with orbital periods of d, d, d and d, respectively. The hosts are main sequence K dwarfs with masses of , , , and and with -band magnitudes of , , and . The Super-Neptune HATS-72b (a.k.a.\ WASP-191b and TOI 294.01) was independently identified as a transiting planet candidate by the HATSouth, WASP and TESS surveys, and we present a combined analysis of all of the data gathered by each of these projects (and their follow-up programs). An exceptionally precise mass is measured for HATS-72b thanks to high-precision radial velocity (RV) measurements obtained with VLT/ESPRESSO, FEROS, HARPS and Magellan/PFS. We also incorporate TESS observations of the warm Saturn-hosting systems HATS-47 (a.k.a. TOI 1073.01), HATS-48A and HATS-49. HATS-47 was independently identified as a candidate by the TESS team, while the other two systems were not previously identified from the TESS data. The RV orbital variations are measured for these systems using Magellan/PFS. HATS-48A has a resolved neighbor in Gaia~DR2, which is a common-proper-motion binary star companion to HATS-48A with a mass of and a current projected physical separation of 1,400 au.

Accepted for publication in AJ. 32 pages, 14 figures, 7 tables