No Transits of Proxima Centauri Planets in High-Cadence TESS Data
Emily A. Gilbert, Thomas Barclay, Ethan Kruse, Elisa V. Quintana, and, Lucianne M. Walkowicz

TL;DR
This study uses high-cadence TESS data and a novel stellar activity modeling method to search for transits of Proxima Centauri planets, concluding that Proxima Centauri b and other Habitable Zone planets are unlikely to transit.
Contribution
The paper introduces a new approach to account for stellar activity in transit searches, improving the reliability of non-detection results for Proxima Centauri planets.
Findings
No transits of Proxima Centauri b detected in TESS data.
Proxima Centauri b cannot be larger than 0.4 Earth radii if transiting.
Likely no Habitable Zone planets larger than Mars transit Proxima Centauri.
Abstract
Proxima Centauri is our nearest stellar neighbor and one of the most well-studied stars in the sky. In 2016, a planetary companion was detected through radial velocity measurements. Proxima Centauri b has a minimum mass of 1.3 Earth masses and orbits with a period of 11.2 days at 0.05 AU from its stellar host, and resides within the star's Habitable Zone. While recent work has shown that Proxima Centauri b likely does not transit, given the value of potential atmospheric observations via transmission spectroscopy of the closest possible Habitable Zone planet, we reevaluate the possibility that Proxima Centauri b is a transiting exoplanet using data from the Transiting Exoplanet Survey Satellite (TESS). We use three sectors (Sectors 11, 12, and 38 at 2-minute cadence) of observations from TESS to search for planets. Proxima Centauri is an extremely active M5.5 star, emitting frequent…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
