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Disproving the validated planets K2-78b, K2-82b, and K2-92b

2017/07/25 by J. Cabrera, S. C. C. Barros, David E.J. Armstrong +16
Physics and Astronomy · #Artificial intelligence #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Centroid #Computer science #Exoplanet #Light curve #Physics #Planet #Stars #Stellar, planetary, and galactic studies #astro-ph.EP #astro-ph.IM

paper · pdf · doi:10.1051/0004-6361/201731233

published as A&A 606, A75 (2017) · accepted for publication in A&A

arxiv created 2017/07/25 · openalex created_date 2017/07/31 · openalex publication_date 2017/07/31 · arxiv updated 2017/10/18 · openalex updated_date 2026/08/05

Abstract

Context. Transiting super-Earths orbiting bright stars in short orbital periods are interesting targets for the study of planetary atmospheres.

Citations