Poster Open Access
{ "publisher": "Zenodo", "DOI": "10.5281/zenodo.5547910", "author": [ { "family": "Mortier, A" } ], "issued": { "date-parts": [ [ 2021, 10, 4 ] ] }, "abstract": "<p>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's leading efforts to fill and interpret the mass-radius diagram of small planets. <br>\n </p>", "title": "Exploring the variety of small planets with HARPS-N", "type": "graphic", "id": "5547910" }
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