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	Monday, October 28, 2024
09:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00	›9:00 (1h) Registration 9:00 - 10:00 (1h) Registration Tea ›10:00 (45min) Introduction François Levrier & Valentine Wakelam › Agora 10:00 - 10:45 (45min) Introduction Agora François Levrier & Valentine Wakelam ›10:45 (1h30) Observations Chair: Pierre Guillard › Agora 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 (1h45) Lunch › Badiane 12:15 - 14:00 (1h45) Lunch Badiane ›14:00 (1h30) Observations Chair: Julien Montillaud › Agora 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 (30min) Tea break › Badiane + Cloitre 15:30 - 16:00 (30min) Tea break Badiane + Cloitre ›16:00 (1h20) Observations Chair: Emeric Bron › Agora 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 (20min) Models Chair: Emeric Bron › Agora 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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