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The discovery of extra-solar planets (exoplanets) has been a staggering advance in astronomy in the last two decades. We have now know that the diversity of planetary systems is far my diverse than we could have even dreamed about. My current interests are understanding how close-in super-earth/mini-neptunes formed and evolve. The origin of these planets which orbit their stars with periods from hours to several months is one of the most interesting puzzles to have arisen from NASA's Kepler mission. The fact that these planets reside so close to their stars also means their atmospheres are subject to intense irradiation, orders of magnitude above what our solar system planets experience. This irradiation drives vigorous atmospheric escape, "evaporating" planets over there long lifetime. By understanding how exoplanet atmosphere's escape we can build a picture of what the planets looked like in the past, gaining insights into how they formed.
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 2 (2024): 1249-1263
arxiv(2024)
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 3 (2024): 5117-5130
ASTRONOMICAL JOURNALno. 2 (2024): 84
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 1 (2023): 385-403
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M. Damasso, J. Rodrigues, A. Castro-González, B. Lavie, Jeanne Davoult,M. R. Zapatero Osorio, Jie Dou, S. G. Sousa,James E. Owen, Paolo A. Sossi, V. Adibekyan,H. Osborn,
arXiv (Cornell University) (2023)
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arXiv (Cornell University)no. 1 (2023): L11-L11
ASTROPHYSICAL JOURNAL LETTERSno. 1 (2023)
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