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Examining TESS light-curve to sort out SOPHIE planetary candidates

neda heidari - Department of Physics, Shahid Beheshti University, Tehran, Iran./Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France (PhD student)

Poster 1

Since stellar activity is a dominant source of noise in both photometric and radial velocity (RV) surveys, a deeper understanding of its effects is essential for accurate exoplanet detection and characterization.  Photometric data of Transiting Exoplanet Survey Satellite (TESS) offers us a unique opportunity to investigate the radial velocity jitters induced by stellar activities through photometric variabilities. In this project, we used the SOPHIE RV measurements and TESS photometry data in order to 1) evaluate the activity of the host star of the SOPHIE planet candidates; 2) investigate the likely activity-induced RV variations; 3) try to detect a new planet …

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