The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations
Context. Characterizing the relation between stellar photometric variability and radial velocity (RV) jitter can help us to better understand the physics behind these phenomena. The current and upcoming high precision photometric surveys such as TESS, CHEOPS, and PLATO will provide the community with thousands of new exoplanet candidates. As a
Hojjatpanah, S. et al.
Fecha de publicación:
7
2020