Jake T. Clark

TL;DR: In this paper, the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stab1242

TL;DR: In this paper, the authors reported observations of a planet transiting AU Microscopii (AU Mic b), which has an orbital period of 846 days, an orbital distance of 007-astronomical units, a radius of 04-Jupiter radii, and a mass of less than 18 Jupiter masses at 3σ confidence.

TL;DR: In this paper, the authors analyze the TESS observations, using novel methods to model and remove instrumental systematic errors, and combine these data with follow-up observations taken from a suite of ground-based telescopes to characterize the planetary system.

TL;DR: The MINERVA-Australis telescope array as discussed by the authors is dedicated to the follow-up, confirmation, characterization, and mass measurement of planets orbiting bright stars discovered by the Transiting Exoplanet Survey Satellite (TESS).

TL;DR: In this paper, the authors reported the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS).