Unifying Galactic and Extragalactic Views of Star Formation - Spectroscopic Studies & Data Science.

9:00 - 10:30 (1h30)

Session 3

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)

10:30 - 11:00 (30min)

Coffee break

Forum de l'Institut d'Astrophysique de Paris (2nd floor)

11:00 - 12:40 (1h40)

Session 4

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)

12:40 - 14:00 (1h20)

Lunch

Cantine de l'Observatoire de Paris

14:00 - 15:40 (1h40)

Session 5

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)

15:40 - 16:10 (30min)

Coffee break

Forum de l'Institut d'Astrophysique de Paris (2nd floor)

16:10 - 17:20 (1h10)

Session 6

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)

Planning