| Oct/2013 | Denver, USA | 45th Division of Planetary Sciences meeting | A new model for volatiles transport in disks |
| Nov/2013 | European Space Agency | Connecting cometary surfaces and interiors | A new model for volatiles transport in disks |
| June/2014 | Paris, France | French Astronomical Society meeting | Origins of the D/H ratio in Neptune |
| Oct/2014 | Lisbon, Portugal | European Planetary Sciences Conference | Origins of the D/H ratio in Neptune |
| Nov/2014 | Cornell University | Invited talk | Formation of carbon-rich planets |
| Nov/2014 | Tucson, Arizona | 46th Division of Planetary Sciences meeting | Formation of carbon-rich planets |
| Nov/2015 | Maryland, USA | 47th Division of Planetary Sciences meeting | Origins of D/H ratio diversity in chondrites |
| March/2016 | Duisburg, Germany | Planets formation and evolution | A pebble accretion model with chemistry |
| Sept/2016 | Baltimore, USA | Linking exoplanet and disk compositions | A pebble accretion model with chemistry |
| July/2016 | Davos, Switzerland | Exoplanets I | C/O ratios of hot Jupiters |
| Oct/2016 | Pasadena, California | 48th Division of planetary sciences meeting | C/O ratios of hot Jupiters |
| Nov/2016 | Toulouse, France | Comets after Rosetta | A pebble accretion model with chemistry |
| March/2017 | Puerto Montt, Chile | Astrochemistry VII | C/O ratios of hot Jupiters |
| July/2017 | University of Cambridge | Invite-only meeting on giant planets chemistry | Can Jupiter be reconciled with Exoplanets ? |
| Nov/2017 | European Space Agency | Invited talk | Connecting the chemistry of planets to protoplanetary disks |
| Feb/2018 | University of Zurich | Water during planet formation | Do planets form preferentially on snowlines ? |
| July/2018 | University of Cambridge | Exoplanets 2 | Is pebble accretion self-limiting ? |
| Feb/2019 | Marseille, France | In situ exploration of ice giants | What is Neptune's D/H ratio telling us about its water abundance ? |
| Feb/2019 | Rostock, Germany | Planet formation conference | Is pebble accretion self-limiting ? |
| May/2019 | Victoria, Canada | New Horizons in Planetary Systems | A color-eccentricity correlation in the Kuiper Belt |
| Oct/2019 | Okinawa, Japan | RESCEU 2019 | Is pebble accretion self-limiting ? |
| Jan/2020 | European Space Agency | Invited talk | Identifying craters with Machine Learning |
| July/2020 | Virtual | Exoplanets 3 | Role of entropy advection in the formation of super Earths |
| Oct/2020 | Virtual | European Planetary Science Conference | Role of entropy advection in the formation of super Earths |
| Nov/2020 | Virtual | PLATO ESP | Role of entropy advection in the formation of super Earths |
| March/2021 | Virtual, Carnegie Institution for Science | Invited talk | How not to make planets |
| Sept/2021 | Virtual | Chemical processes in Solar-type star forming regions | A correlation between the chemistry and eccentricity of hot TNOs |
| Oct/2021 | Virtual | 53rd Division for Planetary Sciences Meeting | A correlation between the chemistry and eccentricity of hot TNOs |
| Nov/2021 | Mohammed Bin Rashid Space Centre | Emirates Lunar Rover science operations team meeting | Mapping ELM's landing zone craters with machine learning |
| April/2022 | Florence, Italy | Atmospheres | Primordial atmospheres are fragile to collisions |
| June/2022 | European Space Agency | Planetary science informatics and data analytics conference | Mapping 67P/C-G boulders with machine learning |
