Morning session
Billy Edwards
University College London (UK)
The Pursuit of a Meticulous Chemical Survey of Exoplanet Atmospheres
Emilie Panek
IAP – CNRS Sorbonne Université (France)
New retrievals from HST observations focusing on the chemistry of exoplanets
Lorenzo Pino
INAF – Osservatorio Astrofisico di Arcetri (Italy)
Ultra-hot Jupiters as laboratories for theories of atmospheric structure and planet formation
Giovanna Tinetti
University College London (UK)
Remote-sensing observations of exo-atmospheres in our galaxy
Patricio E. Cubillos
INAF – Osservatorio Astrofisico di Torino (Italy)
Warm-Jupiter Exoplanet Observations as Probes for Atmospheric Chemical Processes
Amélie Gressier
LATMOS – CNRS (France)
Population study: exploring the transition from super-Earth to sub-Neptune with Hubble transmission survey
Evert Nasedkin
Max Planck Institute for Astronomy (Germany)
Four-of-a-kind: Exploring the atmospheres of the HR 8799 system with GRAVITY
Jack W. Skinner
Queen Mary University of London (UK)
Modons and Other Storms on Hot Exoplanets
Afternoon Session
Renyu Hu
NASA – Jet Propulsion Laboratory (USA)
Toward the Observational Studies of Exoplanet Habitability
Lorenzo Biasiotti
Università degli Studi di Trieste (Italy)
EOS-ESTM: a flexible climate model for habitable exoplanets
Paolo Simonetti
Università degli Studi di Trieste (Italy)
EOS: a new dawn on radiative transfer for habitable worlds
Mohamad Ali-Dib
New York University Abu Dhabi (Emirate Abu Dhabi)
The effect of late giant collisions on the atmospheres of protoplanets and the formation of cold sub-Saturns
Thomas Mikal-Evans
Max Planck Institute for Astronomy (Germany)
Mapping day-night variations in the stratosphere of the ultra-hot Jupiter WASP-121 b
Didier Ricard
CNRM (France)
Characteristics and applications of the Meso-NH mesocale model applied to the Earth atmosphere
Samantha Melani
CNR IBE (Italy)
Data Assimilation in atmospheric models: from operational applications to the impact assessment of future satellite measurements
Stefano Della Fera
Università degli Studi di Bologna (Italy)
The use of spectrally resolved observed radiances to test and improve the representation of the Earth’s atmosphere in climate models
Alfredo Biagini
Università degli Studi di Palermo (Italy)
Stellar activity through simultaneous multiband photometry: V1298 Tau case only