Document Type

Article

Publication Date

5-22-2021

Published In

Monthly Notices Of The Royal Astronomical Society

Abstract

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 Vdwarf star. Photometry from TESS yields radii of Rb = 2.33 ± 0.10 R⊕ and Rc = 2.82 ± 0.15 R⊕, and periods of 3.13 and 7.49 days 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+1.4−1.5 M⊕ and Mc =11.8+3.4−3.2 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.

Keywords

Planetary systems, planets and satellites: individual: TOI-1260b, c, planets and satellites: atmospheres, planets and satellites: composition, techniques: photometric, techniques: radial velocities, stars: low-mass

Comments

This article has been published in Monthly Notices of the Royal Astronomical Society. © 2021 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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