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APRIL 20th |
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08:30 |
Registration |
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10:00 |
Welcome |
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10:20 |
Bianca Maria Dinelli |
CNR-ISAC, Italy |
Analysis of Spectroscopic Observations of the Earth Atmospheres and of the Atmospheres of Other Planets of the Solar System (Titan and Jupiter) |
11:00 |
Coffee break |
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11:20 |
James Cho |
Flatiron Institute, USA |
Large-Scale Planetary Atmospheric Dynamics “from Above” |
11:40 |
Mark Hammond |
Christ Church, Oxford, UK |
3D atmospheric simulations of the lava planet K2-141b to interpret JWST observations |
12:00 |
Matthäus Schulik |
Imperial College London, UK |
The C/O ratio and its influence on hydrodynamic escape of Super-Earth exoplanets |
12:20 |
Yuichi Ito |
National Astronomical Observatory of Japan |
Photo-evaporation of hot rocky exoplanet |
12:40 |
Angelos Tsiaras |
INAF-Arcetri, Italy |
The legacy of HST/WFC3: a prototype for population studies of exoplanets with JWST and Ariel |
13:00 |
Lunch |
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14:00 |
Dmitri Titov |
ESTEC-ESA, The Netherland |
A new view of Venus |
14:40 |
Alessandro Mura |
INAF-IAPS, Italy |
Oscillations and stability of the Jupiter polar cyclones |
15:00 |
Chiara Castagnoli |
INAF-IAPS, Italy |
Study of Jupiter’s auroral regions through the measurement of the Juno/JIRAM instrument |
15:20 |
Luca Ruiz Lozano |
Royal Observatory of Belgium |
Water ice clouds detection with NOMAD LNO nadir channel on board ExoMars TGO |
15:40 |
Fabrizio Oliva |
INAF-IAPS, Italy |
Martian CO2 ice characterization through ExoMars/TGO NOMAD LNO channel nadir high resolution data |
16:00 |
Coffee break |
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16:20 |
Monica Rainer |
INAF, Osservatorio Astronomico di Brera, Italy |
Mars as an exoplanet |
16:40 |
M. E. Cisneros-González |
Université Catholique de Louvain, Belgium |
Upgrade of ASIMUT-ALVL to model the VIS-NIR Jupiter’s atmosphere spectrum |
17:00 |
Márton Mester |
Universidad Complutense de Madrid, Spain |
Oscillations of the Martian Northern Hemisphere Polar Vortex, a Contour Dynamics Perspective |
17:20 |
Evandro Balbi |
University of Genova, Italy |
The Claritas Fossae Fault System (Mars): a potential enhanced pathway for fluids exchange between the inner planet and the Martian atmosphere |
17:40 |
End oral sessions |
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18:30 |
Welcome drink & |
poster session |
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APRIL 21st |
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09:20 |
Billy Edwards |
University College London, UK |
The Pursuit of a Meticulous Chemical Survey of Exoplanet Atmospheres |
09:40 |
Emilie Panek |
IAP, CNRS Sorbonne Université |
New retrievals from HST observations focusing on the chemistry of exoplanets |
10:00 |
Lorenzo Pino |
INAF-Arcetri, Italy |
Ultra-hot Jupiters as laboratories for theories of atmospheric structure and planet formation |
10:20 |
Quentin Changeat |
University College London, UK |
Towards phase-curve retrieval studies of exoplanets in the era of next-generation telescopes |
10:40 |
Coffee break |
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11:00 |
Giovanna Tinetti |
University College London, UK |
Remote-sensing observations of exo-atmospheres in our galaxy |
11:40 |
Patricio E. Cubillos |
INAF, Osservatorio Astrofisico di Torino, Italy |
Warm-Jupiter Exoplanet Observations as Probes for Atmospheric Chemical Processes |
12:00 |
Amélie Gressier |
LATMOS, CNRS, France |
Population study: exploring the transition from super-earth to sub-neptune with a Hubble transmission survey |
12:20 |
Evert Nasedkin |
Max Plank Institute for Astronomy, Germany |
Four-of-a-kind: Exploring the atmospheres of the HR8799 system with GRAVITY |
12:40 |
Jack W. Skinner |
Queen Mary University of London, U.K |
Modons and Other Storms on Hot Exoplanets |
13:00 |
Lunch |
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14:00 |
Renyu Hu |
JPL, USA |
Toward the Observational Studies of Exoplanet Habitability |
14:40 |
Lorenzo Biasiotti |
Universita’ degli Studi di Trieste |
EOS-ESTM: a flexible climate model for habitable exoplanets |
15:00 |
Paolo Simonetti |
Università di Trieste, Italy |
EOS: a new dawn on radiative transfer for habitable worlds |
15:20 |
Mohamad Ali-Dib |
New York University Abu Dhabi |
The effect of late giant collisions on the atmospheres of protoplanets and the formation of cold sub-Saturns |
15:40 |
Thomas Mikal-Evans |
Max Plank Institute for Astronomy, Germany |
Mapping day-night variations in the stratosphere of the ultrahot Jupiter WASP-121b |
16:00 |
Coffee break |
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16:20 |
Didier Ricard |
CNRM, France |
Characteristics and applications of the Meso-NH mesocale model applied to the Earth atmosphere |
17:00 |
Samantha Melani |
CNR IBE, Italy |
Data Assimilation in atmospheric models: from operational applications to the impact assessment of future satellite measurements |
17:20 |
Stefano Della Fera |
Università di Bologna, Italy |
The use of spectrally resolved observed radiances to test and improve the representation of the Earth’s atmosphere in climate models |
17:40 |
Alfredo biagini |
Università di Palermo, Italy |
Stellar activity through simultaneous multiband photometry: V1298 Tau case study |
18:00 |
End oral sessions |
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20:00 |
Social dinner |
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APRIL 22nd |
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09:00 |
Daniele Locci |
Università di Palermo, Italy |
Extreme ultraviolet and X-rays driven photochemistry of gaseous exoplanets. |
09:20 |
Paulina Wolkenberg |
INAF-IAPS, Italy |
Preliminary results of atmospheric parameters varying with LT around volcanoes from PFS-MEx observations |
09:40 |
Francesco Borsa |
INAF, Osservatorio Astronomico di Brera, Italy |
Transmission spectroscopy of exoplanetary atmospheres at high spectral resolution |
10:00 |
Alessandro Marconi |
Università di Firenze, Italy |
ANDES: the ArmazoNes high Dispersion Echelle Spectrograph for the European Extremely Large Telescope |
10:20 |
Óscar Carrión-González |
Technische Universität Berlin, Germany |
Characterizing the atmospheres of cold and temperate exoplanets with direct imaging observations in reflected starlight |
10:40 |
Coffee break |
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11:00 |
Marcel Snels |
CNR-ISAC, Italy |
How to measure spectra of planetary atmospheres in the laboratory ? |
11:40 |
Nadia Balucani |
Università di Perugia, Italy |
Laboratory investigation on the atmospheric chemistry of Titan waiting for the NASA Dragonfly mission: the formation of unsaturated dinitriles |
12:00 |
Gianmarco Vanuzzo |
Università degli Studi di Perugia |
A laboratory investigation of the reaction N(2D) + benzene and implications for the atmospheric chemistry of Titan |
12:20 |
Stefania Stefani |
INAF-IAPS, Italy |
Planetary Atmosphere Simulation System for Spectroscopy (PASSxS), a laboratory set up used to characterize the optical properties of gases at typical planetary conditions |
12:40 |
Silvia Giulia Danelli |
University of Genova, Italy |
Experimental activity at the atmospheric simulation chamber ChAMBRe |
13:00 |
Lunch |
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14:00 |
Donna Rodgers-Lee |
Trinity College Dublin, Ireland |
Impact of magnetic fields and cosmic rays in the context of star formation and exoplanetary systems |
14:40 |
Shang-Min Tsai |
University of Oxford, UK |
The evolution and stability of CO2-CH4-H2O atmospheres |
15:00 |
Arianna Saba |
University College London, UK |
The transmission spectrum of WASP-17 b from the optical to the near-infrared wavelengths: combining STIS, WFC3 and IRAC datasets |
15:20 |
Eva Herrero Cisneros |
Centro de Astrobiologia Madrid, Spain |
ESPRESSO transmission spectroscopy of WASP-54 b and GJ 436 b |
15:40 |
Hugo Tabernero |
Centro de Astrobiologia Madrid, Spain |
The transmission spectrum of the ultra-hot Jupiter WASP-76b |
16:00 |
Coffee break |
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16:30 |
Round table |
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17:30 |
End |
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