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University of Cambridge > Talks.cam > Exoplanet Seminars > Understanding the stars in our search for another Earth
Understanding the stars in our search for another EarthAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Dr Annelies Mortier. To understand exoplanetary systems, we can study their mass-radius relationship or lack thereof. The HARPS -N Collaboration has been leading the efforts to fill and interpret the mass-radius diagram of small planets by combining space photometry, Gaia astrometry and radial velocities. Determining a precise as-well-as accurate planet mass can only be determined with well-sampled, stable, and precise observations combined with advanced computational efforts and new extraction and processing techniques. The biggest challenge remains the stellar activity processes, mimicking and hiding planetary signals. With the HARPS -N Collaboration, we have been studying the Sun-as-a-star for 6 years, providing a dataset where we truly have no planetary signals and can study stellar behaviour in more detail. In this talk, I will give an overview on the leading efforts of our collaboration to fill the mass-radius diagram, an insight in new LSD -based processing techniques, and the behaviour over time of the standard activity indicators using Solar data. This talk is part of the Exoplanet Seminars series. This talk is included in these lists:
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