CORDIS Project
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This project focuses on detecting low-mass companions around stars using space mission data. By employing a novel algorithm, it aims to identify new massive planets and brown dwarfs, enhancing our understanding of planetary systems and their formation.
I propose to lead an international observational effort to characterize the population of massive planets, brown dwarf and stellar secondaries orbiting their parent stars with short periods, up to 10-30 days.
The effort will utilize the superb, accurate, continuous lightcurves of more than hundred thousand stars obtained recently by two space missions – CoRoT and Kepler. I propose to use these lightcurves to detect non-transiting low-mass companions with a new algorithm, BEER, which I developed…
TEL AVIV UNIVERSITY
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