CORDIS Project
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This project focuses on improving the detection of exoplanets through radial velocity measurements. It aims to develop methods to separate planetary signals from stellar activity, enhancing the accuracy of future exoplanet surveys.
Radial velocity (RV) planet searches are a key exoplanet detection method, and one of the only ways to measure a planet's mass.
The best RV instruments today reach precisions well below 1 m/s, something which would have seemed impossible 30 years ago.
The key factor limiting the sensitivity of RV surveys now is stellar activity.
Regions of enhanced magnetic flux on the stellar surface alter the shape of absorption lines in the stellar spectrum, and perturb the measured RVs. I have developed phys…
THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD
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