October 4, 2021 Poster Open Access

Mortier, A

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    <subfield code="a">&lt;p&gt;To understand exoplanetary systems, we can study their mass-radius relationship or lack thereof. Kepler, K2, and TESS discover thousands of exoplanet candidates providing precise transit photometry which are then followed up by ground-based spectroscopy to characterise their masses and internal composition. The expertise gained from this process will be invaluable for the PLATO mission when pushing to longer-period small planets. In this poster, I give an overview of the HARPS-N Collaboration&amp;#39;s leading efforts to fill and interpret the mass-radius diagram of small planets.&amp;nbsp;&lt;br&gt;
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