HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity

TL;DR

This paper reports the discovery and characterization of HATS-2b, a transiting exoplanet around a star with starspot activity, providing insights into the planet's properties and stellar activity effects.

Contribution

The study presents the discovery of HATS-2b and detailed analysis of starspot activity on its host star using multi-band transit photometry.

Findings

HATS-2b has a mass of 1.37 M_J and radius of 1.14 R_J.

The host star shows significant starspot activity.

Transit light curves reveal anomalies consistent with starspots.

Abstract

We report the discovery of HATS-2b, the second transiting extrasolar planet detected by the HATSouth survey. HATS-2b is moving on a circular orbit around a V=13.6 mag, K-type dwarf star (GSC 6665-00236), at a separation of 0.0230 \pm 0.0003 AU and with a period of 1.3541 days. The planetary parameters have been robustly determined using a simultaneous fit of the HATSouth, MPG/ESO~2.2\,m/GROND, Faulkes Telescope South/Spectral transit photometry and MPG/ESO~2.2\,m/FEROS, Euler~1.2\,m/CORALIE, AAT~3.9\,m/CYCLOPS radial-velocity measurements. HATS-2b has a mass of 1.37 \pm 0.16 M_J, a radius of 1.14 \pm 0.03 R_J and an equilibrium temperature of 1567 \pm 30 K. The host star has a mass of 0.88 \pm 0.04 M_Sun, radius of 0.89 \pm 0.02 R_Sun and shows starspot activity. We characterized the stellar activity by analysing two photometric follow-up transit light curves taken with the GROND instrument, both obtained simultaneously in four optical bands (covering the wavelength range of 3860-9520 \AA). The two light curves contain anomalies compatible with starspots on the photosphere of the parent star along the same transit chord.