Monday, October 28, 2024

Time Event (+)
09:00 - 10:00 Registration - Tea  
10:00 - 10:45 Introduction (Agora) - François Levrier & Valentine Wakelam  
10:45 - 12:15 Observations (Agora) (+)  
10:45 - 11:15 › Highlights from the Galactic Cold Cores Program - Isabelle Ristorcelli, Institut de recherche en astrophysique et planétologie  
11:15 - 11:35 › 3D extinction mapping of the Milky Way with the Besançon Galaxy Model in the Gaia era - Barnabé DEFORET, Institut UTINAM  
11:35 - 11:55 › Highlights of the SOFIA Legacy Program FEEDBACK - Nicola Schneider, University of Cologne  
11:55 - 12:15 › The High/Intermediate velocity HI cloud population of the Small Magellanic Cloud - Frances Buckland-Willis, Laboratoire de physique de l'ENS - ENS Paris  
12:15 - 14:00 Lunch (Badiane)  
14:00 - 15:30 Observations (Agora) (+)  
14:00 - 14:30 › The physics of molecular hydrogen in space with JWST - Pierre Guillard, Institut d'Astrophysique de Paris, Sorbonne Université  
14:30 - 14:50 › The Long-Wavelength Dust Properties of Nearby Galaxies, probed by NIKA2 - Frédéric Galliano, Astrophysique Interprétation Modélisation  
14:50 - 15:10 › The radio view of diffuse molecular gas - Harvey Liszt, National Radio Astronomy Observatory  
15:10 - 15:30 › An information-theory based method to determine the best emission lines to constrain the physical conditions of interstellar clouds - Emeric Bron, Observatoire de Paris  
15:30 - 16:00 Tea break (Badiane + Cloitre)  
16:00 - 17:20 Observations (Agora) (+)  
16:00 - 16:20 › Estimating the dust-heating interstellar radiation field in nearby galaxies using the PHANGS MUSE+JWST+ASTROSAT surveys - Raphael Maris, IRAP  
16:20 - 16:40 › 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  
16:40 - 17:00 › Scattering Transforms and component separation for ISM Physics - Erwan Allys, Laboratoire de physique de l'ENS - ENS Paris  
17:00 - 17:20 › Infrared signatures from multiple chemistries in the d203-504 protoplanetary disk - Ilane Schroetter, Institut de recherche en astrophysique et planétologie  
17:20 - 17:40 Models (Agora) (+)  
17:20 - 17:40 › Modeling the chemical impacts of luminosity outbursts in protostellar envelopes - Antoine Espagnet, Institut de recherche en astrophysique et planétologie  

Tuesday, October 29, 2024

Time Event (+)
09:00 - 10:30 Laboratory Astrophysics (Agora) (+)  
09:00 - 09:30 › Unveiling new reactive species of astrophysical relevance using laboratory rotational spectroscopy: the case of the H2NCO radical - Marie-Aline Martin-Drumel, Institut des Sciences Moléculaires d'Orsay  
09:30 - 09:50 › Differential reactivity of the [CHO]+ isomers - Nicolas SOLEM, Institut de Chimie Physique  
09:50 - 10:10 › Flux and fluence effects on the Vacuum-UV photodesorption and photoprocessing of CO2 ices - ANTOINE HACQUARD, MONARIS, De la Molécule aux Nanos-objets : Réactivité, Interactions et Spectroscopies, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères  
10:10 - 10:30 › Laboratory experiments to understand the molecular diversity of astrophysical environments - Grégoire Danger, Physique des interactions ioniques et moléculaires  
10:30 - 11:00 Tea break (Badiane + Cloitre)  
11:00 - 12:30 Laboratory Astrophysics (Agora) (+)  
11:00 - 11:30 › Photodesorption from interstellar ice analogues: what do we currently know from laboratory experiments - Mathieu Bertin, MONARIS, De la Molécule aux Nanos-objets : Réactivité, Interactions et Spectroscopies  
11:30 - 11:50 › Manoeuvring chemical reactions one degree of freedom at a time - Jutta Toscano, University of Basel  
11:50 - 12:10 › Sticking Coefficients of Astrochemically-Relevant Ices on Realistic Grains Analogues are Lower than Expected - Caroline Stadler, CINaM  
12:10 - 12:30 › Studying the VUV photoprocessing of superhydrogenated PAHs and the structure of PAH-water clusters in astro-relevant conditions - Alexandre Marciniak, Laboratoire Collisions Agrégats Réactivité, Institut de recherche en astrophysique et planétologie  
12:30 - 14:00 Lunch (Badiane)  
14:00 - 14:30 Laboratory Astrophysics (Agora) (+)  
14:00 - 14:30 › Spectroscopic properties of cosmic dust analogues to support the interpretation of astronomical data - Karine Demyk, Institut de recherche en astrophysique et planétologie  
14:30 - 15:10 Observations (Agora) (+)  
14:30 - 14:50 › Carbon chain molecules towards massive clumps: the cold envelope still has surprises! - Laure Bouscasse, IRAM  
14:50 - 15:10 › Detections of Carbon Radio Recombination Lines with the NenuFAR telescope - Lucie Cros, LPENS  
15:10 - 15:30 Models (Agora) (+)  
15:10 - 15:30 › Modeling the neutral gas heating in low metallicity galaxies - Maxime Varese, Université Paris-Cité, Université Paris-Saclay, CEA  
15:30 - 16:20 Tea break + Poster session (Badiane + Cloitre)  
16:20 - 16:40 Models (Agora) (+)  
16:20 - 16:40 › On the impact of atomic and molecular accretion on interstellar dust growth - Duncan Bossion, Institut de Physique de Rennes  
16:40 - 17:00 Observations (Agora) (+)  
16:40 - 17:00 › Understanding the Star Formation Efficiency in Dense Gas with the CAFFEINE ArTéMiS survey - Michael Mattern, Laboratoire d'Astrophysique (AIM)  
17:00 - 17:20 Models (Agora) (+)  
17:00 - 17:20 › Towards robust estimations of molecular cloud physical conditions from multi-species lines: The case of the Horsehead nebula - Léontine Ségal, Institut Matériaux Microélectronique et Nanosciences de Provence, Université de Toulon  
20:00 - 22:00 Conférence grand public - TBD (Agora) - Nathalie Brouillet (LAB)  

Wednesday, October 30, 2024

Time Event (+)
09:00 - 10:30 Laboratory Astrophysics (Agora) (+)  
09:00 - 09:30 › Molecular collisions in the interstellar medium: successes and challenges - Jérome Loreau, Department of Chemistry [Leuven]  
09:30 - 09:50 › Nuclear-spin astrochemistry: from laboratory to observations - Alexandre Faure, Institut de Planétologie et d'Astrophysique de Grenoble  
09:50 - 10:10 › Towards non-LTE modelling of large interstellar cyclic species: the collisional excitation of cyclopentadiene - Sándor Demes, Institut de Physique de Rennes  
10:10 - 10:30 › Dissociative recombination of NS+ in collision with low-energy electrons - Riyad Hassaine, LOMC, Univ. Le Havre Normandie  
10:30 - 11:00 Tea break (Badiane + Cloitre)  
11:00 - 11:20 Models (Agora) (+)  
11:00 - 11:20 › Collisional excitation of PO+ by para-H2: towards the accurate modeling of phosphorus abundance in the ISM - Francesca Tonolo, Dipartimento di Chimica "Giacomo Ciamician", Università di Bologna  
11:20 - 11:50 Observations (Agora) (+)  
11:20 - 11:50 › La physico-chimie des disques protoplanétaires à l'ère du JWST - Benoît Tabone, Institut d'astrophysique spatiale  
11:50 - 12:30 Laboratory Astrophysics (Agora) (+)  
11:50 - 12:10 › Investigating the photophysics and isomerization of C11H9+ - Lozano Ana I., Institut de Recherche en Astrophysique et Planétologie (IRAP)  
12:10 - 12:30 › Rapid molecular growth induced by low-temperature ion-molecule reactions of CH3+ with a selection of hydrocarbons : insights into the interstellar carbon chemistry - Elliot Ogden, Institut de Physique de Rennes  
12:30 - 14:00 Lunch (Badiane)  
14:00 - 14:50 Laboratory Astrophysics (Agora) (+)  
14:00 - 14:30 › Rate constants and product yields of astrochemically relevant reactions: Experiment and theory - Kevin Hickson, Institut des Sciences Moléculaires  
14:30 - 14:50 › Collision-induced dynamics of PAH-water clusters - Héloïse Leboucher, Laboratoire de Chimie et Physique Quantiques  
14:50 - 15:30 Observations (Agora) (+)  
14:50 - 15:10 › Study of cosmic-ray acceleration regions through their chemical composition - Aimie Clément, Laboratoire de Physique des Deux Infinis Bordeaux, Laboratoire d'Astrophysique de Bordeaux  
15:10 - 15:30 › Magnetic fields and first results on the ionization fraction in Orion B - Ivana Beslic, LERMA, Observatoire de Paris  
18:00 - 21:00 Social Event  

Thursday, October 31, 2024

Time Event (+)
09:00 - 10:10 Observations (Agora) (+)  
09:00 - 09:30 › Emerging molecular complexity towards high-mass protostellar envelopes - Timea Csengeri, Laboratoire d'Astrophysique de Bordeaux  
09:30 - 09:50 › New molecules and isotopologues discovered with the QUIJOTE line survey - José Cernicharo, Instituto de Física Fundamental [Madrid]  
09:50 - 10:10 › Anatomy of the Class I protostar L1489 IRS with NOEMA at 3mm - Maxime Tanious, Institut de Planétologie et d'Astrophysique de Grenoble  
10:10 - 10:30 Models (Agora) (+)  
10:10 - 10:30 › Toward the detection of the sulphur reservoir(s) in the JWST era ? - Angèle Taillard, Centro de Astrobiologia [Madrid]  
10:30 - 11:00 Tea break (Badiane + Cloitre)  
11:00 - 12:20 Observations (Agora) (+)  
11:00 - 11:20 › Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) - Audrey Coutens, Institut de recherche en astrophysique et planétologie  
11:20 - 11:40 › Complex organic molecules detected in hot cores with machine learning - Nina Kessler, Laboratoire d'Astrophysique de Bordeaux  
11:40 - 12:00 › Sulphur-bearing species trace ongoing star formation in the Central Molecular Zone of NGC 253 - Mathilde Bouvier, Leiden Observatory  
12:00 - 12:20 › On-going gas-phase organic chemistry observed through the emission of CH+ and CH3+ in the Orion Bar - Marion ZANNESE, Institut d'Astrophysique Spatiale