Monday, October 28, 2024 › | |
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
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›9:00 (1h)
9:00 - 10:00 (1h)
Registration
Tea
10:00 - 10:45 (45min)
Introduction
Agora
François Levrier & Valentine Wakelam
10:45 - 12:15 (1h30)
Observations
Agora
Chair: Pierre Guillard
› Highlights from the Galactic Cold Cores Program
- Isabelle Ristorcelli, Institut de recherche en astrophysique et planétologie
10:45-11:15 (30min)
› 3D extinction mapping of the Milky Way with the Besançon Galaxy Model in the Gaia era
- Barnabé DEFORET, Institut UTINAM
11:15-11:35 (20min)
› Highlights of the SOFIA Legacy Program FEEDBACK
- Nicola Schneider, University of Cologne
11:35-11:55 (20min)
› The High/Intermediate velocity HI cloud population of the Small Magellanic Cloud
- Frances Buckland-Willis, Laboratoire de physique de l'ENS - ENS Paris
11:55-12:15 (20min)
12:15 - 14:00 (1h45)
Lunch
Badiane
14:00 - 15:30 (1h30)
Observations
Agora
Chair: Julien Montillaud
› The physics of molecular hydrogen in space with JWST
- Pierre Guillard, Institut d'Astrophysique de Paris, Sorbonne Université
14:00-14:30 (30min)
› The Long-Wavelength Dust Properties of Nearby Galaxies, probed by NIKA2
- Frédéric Galliano, Astrophysique Interprétation Modélisation
14:30-14:50 (20min)
› The radio view of diffuse molecular gas
- Harvey Liszt, National Radio Astronomy Observatory
14:50-15:10 (20min)
› An information-theory based method to determine the best emission lines to constrain the physical conditions of interstellar clouds
- Emeric Bron, Observatoire de Paris
15:10-15:30 (20min)
15:30 - 16:00 (30min)
Tea break
Badiane + Cloitre
16:00 - 17:20 (1h20)
Observations
Agora
Chair: Emeric Bron
› Estimating the dust-heating interstellar radiation field in nearby galaxies using the PHANGS MUSE+JWST+ASTROSAT surveys
- Raphael Maris, IRAP
16:00-16:20 (20min)
› Why sub-mm dust continuum emission is not a faithful tracer of the nature of faint filaments in molecular clouds
- Pierre Hily-Blant, IPAG, Université Grenoble Alpes
16:20-16:40 (20min)
› Scattering Transforms and component separation for ISM Physics
- Erwan Allys, Laboratoire de physique de l'ENS - ENS Paris
16:40-17:00 (20min)
› Infrared signatures from multiple chemistries in the d203-504 protoplanetary disk
- Ilane Schroetter, Institut de recherche en astrophysique et planétologie
17:00-17:20 (20min)
17:20 - 17:40 (20min)
Models
Agora
Chair: Emeric Bron
› Modeling the chemical impacts of luminosity outbursts in protostellar envelopes
- Antoine Espagnet, Institut de recherche en astrophysique et planétologie
17:20-17:40 (20min)
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Session | Speech | Logistics | Break | Tour |