Amphithéâtre de l'Institut d'Astrophysique de Paris
Romane Le Gal
› Filaments and fibers in the Gould Belt molecular clouds - Alvaro Hacar, University of Vienna
14:00-14:30 (30min)
› Understanding the dynamical state of star-forming filaments through magnetic field morphology: First results from the B-FUN project with NIKA2-POL -
14:30-14:50 (20min)
› Tracing Variations of Dust Emissivity Spectral Index Associated with Interstellar Shocks - Wonju Kim, Max-Planck-Institut für Radioastronomie
14:50-15:10 (20min)
› ALMA-IMF - Frédérique Motte, Institut de Planétologie et d'Astrophysique de Grenoble
15:10-15:40 (30min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Antoine Zakardjian
› A High-Resolution View of Dense Gas Across Galactic Environments: Insights from M51 and Beyond - Sophia Stuber, National Astronomical Observatory of Japan, Max Planck Institute for Radio Astronomy
09:00-09:30 (30min)
› Connecting Star Formation in the Milky Way and Nearby Galaxies -- Consistency of Star Formation on Molecular-Cloud Scales Across Galaxies - Jianwen Zhou, Max Planck Institute for Radio Astronomy
09:30-09:50 (20min)
› Bayesian modeling of the multiphase ISM of a star- forming region in the LMC - Léo Belloir, Astrophysique Interprétation Modélisation
09:50-10:10 (20min)
› Hierarchical Bayesian modeling of the spatially-resolved ISM in the nearby galaxy M99 - Frédéric Galliano, UMR Astrophysique, Instrumentation-Modelisation, à Paris-Saclay
10:10-10:30 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Ivana Beslic
› Multi-line observations of nearby galaxies - Antonio Usero, Observatorio Astronomico Nacional (IGN)
11:00-11:30 (30min)
› Comparative lifetime of atomic and molecular clouds in nearby galaxies - Lise Ramambason, Heidelberg University
11:30-12:00 (30min)
› Topological models to recover intrinsic variations of physical conditions in galaxies - Vianney Lebouteiller, Astrophysique Interprétation Modélisation - Maxime Varese, Astrophysique Interprétation Modélisation
12:00-12:20 (20min)
› LEGO: A Comprehensive Imaging Line Survey of Galactic Molecular Clouds - Jens Kauffmann, Haystack Observatory, Massachusetts Institute of Technology
12:20-12:40 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Antonio Usero
› Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations -
14:00-14:30 (30min)
› LEGO: Connecting Probes of Dense Gas from the Milky Way to External Galaxies - Lukas Neumann, European Southern Observatory
14:30-14:50 (20min)
› Multi-species non-LTE modelling of Galactic massive star forming regions - Minou Greve, Argelander Institut fur Astronomie
14:50-15:10 (20min)
› Revisiting the role of the HCN(1-0) line as a tracer of the dense gas reservoir for star formation. - Miriam G. Santa-Maria, Instituto de Física Fundamental [Madrid]
15:10-15:40 (30min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Mario Tafalla
› Application of scattering transforms to the separation of ISM phases - Erwan Allys, Laboratoire de physique de l'ENS - ENS Paris
16:10-16:40 (30min)
› Fitting AGN and host galaxy emission lines with CIGALE - Patrice Theule, Laboratoire d'Astrophysique de Marseille
16:40-17:00 (20min)
› Beyond Moment 0: Deep Learning the Spectral Kinematics of High-z Star Formation? - Arnab Lahiry, Foundation for Research and Technology - Hellas, University of Crete [Heraklion]
17:00-17:20 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Karine Demyk
› Magnetic field and star formation - Anaëlle Maury, ICE/CSIC & CEA/AIM
09:00-09:30 (30min)
› A model for late accretion streamers and chemical replenishment in protoplanetary disks - David Navarro, Centro de Astrobiologia
09:30-09:50 (20min)
› Grain growth in the early stage of star formation revealed by NIKA2 observations and 3D radiative transfer modeling - Enyi Zhu, Institut de recherche en astrophysique et planétologie
09:50-10:10 (20min)
› Gas-phase Elemental abundances in Molecular CloudS (GEMS): Understanding the diversity of starless cores. - Fuente Asuncion, Centro de Astrobiologia (CAB, CSIC-INTA)
10:10-10:30 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Lucas Einig
› Flow Matching for Robust Simulation-Based Inference under Model Misspecification - Florence Forbes, Centre Inria de l'Université Grenoble Alpes, Modèles statistiques bayésiens et des valeurs extrêmes pour données structurées et de grande dimension
11:00-11:30 (30min)
› Toward robust estimates of the physicochemical properties of interstellar molecular clouds without ground truth - Léontine Ségal, Thales LAS France
11:30-12:00 (30min)
› Chemical complexity in outer Galaxy star-forming regions - Francesco Fontani, Laboratoire d'étude de l'Univers et des phénomènes eXtrèmes, INAF - Osservatorio Astrofisico di Arcetri, Center for Astrochemical Studies
12:00-12:20 (20min)
› T|3D Presenting The First 3D-Temperature-Map Of Our Galaxy - Jonathan Shelest, Technion - Israel Institute of Technology [Haifa]
12:20-12:40 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Franck Le Petit
› Neural network-based emulation of ISM models : the case of the Meudon PDR code - Emeric Bron, Laboratoire d'étude de l'Univers et des phénomènes eXtrèmes
14:00-14:30 (30min)
› BEETROOTS, a new bayesian framework for inverse problems, - Pierre Palud, Observatory of Meudon
14:30-15:00 (30min)
› A hierarchical likelihood model for non-linear inverse problems under additive and multiplicative noises - Nicolas Goeman, Centre de Recherche en Informatique, Signal et Automatique de Lille - UMR 9189
15:00-15:20 (20min)
› Deciphering Photodissociation Regions: Radiative Feedback, High-Resolution Infrared Tracers, and Advanced Astrochemical Modeling. - Aurélien Piluso, Observatoire de Paris
15:20-15:40 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Marion Zannesse
› Quantifying the information content of spectral tracers for interstellar medium studies - Lucas Einig, Institut de RadioAstronomie Millimétrique, Grenoble Images Parole Signal Automatique
16:10-16:40 (30min)
› Assisting sampling with generative models - Marylou Gabrié, Département de Physique de l'ENS-PSL
16:40-17:10 (30min)
› Observational study of a hot corino cluster bathed by an external UV radiation field - Aina Palau, Universidad Nacional Autónoma de México = National Autonomous University of Mexico
17:10-17:30 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Pierre Gratier
› Deep priors for approximate posterior sampling in imaging inverse problems - Thomas Oberlin, Institut Supérieur de l'Aéronautique et de l'Espace
09:00-09:30 (30min)
› The fundamental structure and physical conditions of the Orion Bar as seen by JWST and ALMA - Marion Zannese, Instituto de Física Fundamental [Madrid]
09:30-09:50 (20min)
› Identifying the Stellar Populations "behind" interstellar clouds for Ice Mapping the distribution of solid material in star-forming regions - Lorenzo Demaria, The Open University
09:50-10:10 (20min)
› From IR dark clouds to evolved Hii regions: a machine learning approach to identifying evolutionary stages of molecular clumps - Karolina Plakitina, Institute of Astronomy of the Russian Academy of Sciences
10:10-10:30 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Maryvonne Gerin
› The Structure of Nearby Molecular Clouds Revealed by Ammonia - Jaime Pineda, Giessenbachstrasse 1
11:00-11:30 (30min)
› Dense core chemistry - Helena Mazurek, LUX
11:30-12:00 (30min)
› Fusion of JWST data - Demonstrating practical feasibility - Landry Marquis, Institut de recherche en astrophysique et planétologie, Signal et Communications, Institut Supérieur de l'Aéronautique et de l'Espace
12:00-12:20 (20min)
› Resolved CO Isotopologues and Dust Emission in Giant Molecular Clouds of the Andromeda Galaxy - Chloe Bosomworth, Centre for Astrophysics Research [Hatfield]
12:20-12:40 (20min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Olivier Flasseur
› Deep learning for source/line detection in hyperspectral data - David Cornu, LUX
14:00-14:30 (30min)
› Automated line attribution in line surveys - Timea Csengeri, LAB
14:30-15:00 (30min)
› Probing the potential for kinematically colder H I component as a tracer for star-forming gas in nearby galaxies - Hye-Jin Park, Australian National University, CEA Paris-Saclay
15:00-15:20 (20min)
› High-angular resolution, wide-field observations of the Milky Way Central Molecular Zone - Jonathan Henshaw, Max Planck Institute for Astronomy
15:20-15:50 (30min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Antoine Roueff
› Deep learning for radar image processing - Florence Tupin, LTCI, Télécom Paris
16:20-16:50 (30min)
› Exploring the circumstellar environment by direct imaging at high contrast with data-driven approaches - Olivier Flasseur, Centre de Recherche Astrophysique de Lyon
16:50-17:20 (30min)
Amphithéâtre de l'Institut d'Astrophysique de Paris
Timea Csengeri
› From Diffuse Gas to Star-Forming Filaments: Mapping the Magnetic and Ionization Landscape of Orion B - Ivana Beslic, LUX, Observatoire de Paris
09:00-09:30 (30min)
› Direct Detection of Cosmic-Ray-Excited H₂ in Interstellar Space - Shmuel Bialy, Technion - Israel Institute of Technology [Haifa]
09:30-09:50 (20min)
› The cosmic-ray ionization rate in nearby cold clumps - Gan Luo, Institut de RadioAstronomie Millimétrique
09:50-10:10 (20min)
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Amphithéâtre de l'Institut d'Astrophysique de Paris
