› 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)
› 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)
› 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)
› 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
09:00-09:30 (30min)
› Differential reactivity of the [CHO]+ isomers - Nicolas SOLEM, Institut de Chimie Physique
09:30-09:50 (20min)
› 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
09:50-10:10 (20min)
› Laboratory experiments to understand the molecular diversity of astrophysical environments - Grégoire Danger, Physique des interactions ioniques et moléculaires
10:10-10:30 (20min)
› 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
11:00-11:30 (30min)
› Manoeuvring chemical reactions one degree of freedom at a time - Jutta Toscano, University of Basel
11:30-11:50 (20min)
› Sticking Coefficients of Astrochemically-Relevant Ices on Realistic Grains Analogues are Lower than Expected - Caroline Stadler, CINaM
11:50-12:10 (20min)
› 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
12:10-12:30 (20min)
› Spectroscopic properties of cosmic dust analogues to support the interpretation of astronomical data - Karine Demyk, Institut de recherche en astrophysique et planétologie
14:00-14:30 (30min)
› Modeling the neutral gas heating in low metallicity galaxies - Maxime Varese, Université Paris-Cité, Université Paris-Saclay, CEA
15:10-15:30 (20min)
› Understanding the Star Formation Efficiency in Dense Gas with the CAFFEINE ArTéMiS survey - Michael Mattern, Laboratoire d'Astrophysique (AIM)
16:40-17:00 (20min)
› 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
17:00-17:20 (20min)
› Molecular collisions in the interstellar medium: successes and challenges - Jérome Loreau, Department of Chemistry [Leuven]
09:00-09:30 (30min)
› Nuclear-spin astrochemistry: from laboratory to observations - Alexandre Faure, Institut de Planétologie et d'Astrophysique de Grenoble
09:30-09:50 (20min)
› Towards non-LTE modelling of large interstellar cyclic species: the collisional excitation of cyclopentadiene - Sándor Demes, Institut de Physique de Rennes
09:50-10:10 (20min)
› Dissociative recombination of NS+ in collision with low-energy electrons - Riyad Hassaine, LOMC, Univ. Le Havre Normandie
10:10-10:30 (20min)
› 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
11:00-11:20 (20min)
› On-going gas-phase organic chemistry observed through the emission of CH+ and CH3+ in the Orion Bar - Marion ZANNESE, Institut d'Astrophysique Spatiale
11:20-11:40 (20min)
› Investigating the photophysics and isomerization of C11H9+ - Lozano Ana I., Institut de Recherche en Astrophysique et Planétologie (IRAP)
11:40-12:00 (20min)
› 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
12:00-12:20 (20min)
› Rate constants and product yields of astrochemically relevant reactions: Experiment and theory - Kevin Hickson, Institut des Sciences Moléculaires
14:00-14:30 (30min)
› Collision-induced dynamics of PAH-water clusters - Héloïse Leboucher, Laboratoire de Chimie et Physique Quantiques
14:30-14:50 (20min)
› Study of cosmic-ray acceleration regions through their chemical composition - Aimie Clément, Laboratoire de Physique des Deux Infinis Bordeaux, Laboratoire d'Astrophysique de Bordeaux
14:50-15:10 (20min)
› Magnetic fields and first results on the ionization fraction in Orion B - Ivana Beslic, LERMA, Observatoire de Paris
15:10-15:30 (20min)
- ()
› - Audrey Coutens, Institut de recherche en astrophysique et planétologie
11:00-11:20 ()
› - Nina Kessler, Laboratoire d'Astrophysique de Bordeaux
11:20-11:40 ()
› Emerging molecular complexity towards high-mass protostellar envelopes - Timea Csengeri, Laboratoire d'Astrophysique de Bordeaux
09:00-09:30 (30min)
› New molecules and isotopologues discovered with the QUIJOTE line survey - José Cernicharo, Instituto de Física Fundamental [Madrid]
09:30-09:50 (20min)
› Anatomy of the Class I protostar L1489 IRS with NOEMA at 3mm - Maxime Tanious, Institut de Planétologie et d'Astrophysique de Grenoble
09:50-10:10 (20min)
› Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) - Audrey Coutens, Institut de recherche en astrophysique et planétologie
11:00-11:20 (20min)
› Complex organic molecules detected in hot cores with machine learning - Nina Kessler, Laboratoire d'Astrophysique de Bordeaux
11:20-11:40 (20min)
› Sulphur-bearing species trace ongoing star formation in the Central Molecular Zone of NGC 253 - Mathilde Bouvier, Leiden Observatory
11:40-12:00 (20min)