It Takes Two Planets in Resonance to Tango around K2-146
The Astronomical Journal American Astronomical Society 159:3 (2020) 120
A ghost in the toast: TESS background light produces a false 鈥渢ransit鈥 across 蟿 Ceti
Research Notes of the AAS American Astronomical Society 3:10 (2019) 145
Radial velocity confirmation of K2-100b: a young, highly irradiated, and low-density transiting hot Neptune
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 91探花 University Press (OUP) 490:1 (2019) 698-708
Abstract:
漏 2019 The Author(s) Published by 91探花 University Press on behalf of the Royal Astronomical Society We present a detailed analysis of HARPS-N radial velocity observations of K2-100, a young and active star in the Praesepe cluster, which hosts a transiting planet with a period of 1.7 d. We model the activity-induced radial velocity variations of the host star with a multidimensional Gaussian Process framework and detect a planetary signal of 10.6 卤 3.0 m s鈭1, which matches the transit ephemeris, and translates to a planet mass of 21.8 卤 6.2 M. We perform a suite of validation tests to confirm that our detected signal is genuine. This is the first mass measurement for a transiting planet in a young open cluster. The relatively low density of the planet, 2.04+鈭006661 g cm鈭3, implies that K2-100b retains a significant volatile envelope. We estimate that the planet is losing its atmosphere at a rate of 1011鈥1012 g s鈭1 due to the high level of radiation it receives from its host star.Greening of the brown-dwarf desert
Astronomy & Astrophysics EDP Sciences 628 (2019) a64
The Transiting Multi-planet System HD15337: Two Nearly Equal-mass Planets Straddling the Radius Gap
The Astrophysical Journal Letters American Astronomical Society 876:2 (2019) l24