
Judith Korth
Postdoc

Hot planets around cool stars - Two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
Author
Summary, in English
We present the discovery and characterization of two sub-Neptunes in close orbits, as well as a tentative outer planet of a similar size, orbiting TOI-1260 - a low metallicity K6 V dwarf star. Photometry from Transiting Exoplanet Survey Satellite(TESS) yields radii of Rb = 2.33 ± 0.10 and Rc = 2.82 ± 0.15 R⊕, and periods of 3.13 and 7.49 d for TOI-1260 b and TOI-1260 c, respectively. We combined the TESS data with a series of ground-based follow-up observations to characterize the planetary system. From HARPS-N high-precision radial velocities we obtain Mb = 8.6- 1.5+ 1.4 and Mc = 11.8- 3.2+ 3.4 M⊕. The star is moderately active with a complex activity pattern, which necessitated the use of Gaussian process regression for both the light-curve detrending and the radial velocity modelling, in the latter case guided by suitable activity indicators. We successfully disentangle the stellar-induced signal from the planetary signals, underlining the importance and usefulness of the Gaussian process approach. We test the system's stability against atmospheric photoevaporation and find that the TOI-1260 planets are classic examples of the structure and composition ambiguity typical for the 2-3 R⊕ range.
Publishing year
2021-08-01
Language
English
Pages
4684-4701
Publication/Series
Monthly Notices of the Royal Astronomical Society
Volume
505
Issue
4
Document type
Journal article
Publisher
Oxford University Press
Keywords
- planetary systems
- planets and satellites: atmospheres
- planets and satellites: composition
- planets and satellites: individual: TOI-1260b, c
- stars: low-mass
- techniques: photometric
- techniques: radial velocities
Status
Published
ISBN/ISSN/Other
- ISSN: 0035-8711