The daily schedule is typically composed of two informal talks / discussions per day, one in the morning and one in the afternoon, and working sessions in smaller groups the rest of the time.

Week 1

Date Time Place Speaker Topic
Monday, July 3 9:30 209 -- Welcome coffee
10:00 - 11:00 209 Everyone Lightning
11:00 - 12:00 121 Joshua Peek The ISM beyond three dimensions
15:30 - 16:00 209 Gail Zasowski The Diffuse Interstellar Bands: Past and Future
18:00 - 19:00 121 Paris-Saclay + Pascal Institute Welcome reception
Tuesday, July 4 10:00 - 11:00 209 Gregory Green Mapping Dust in 3D with Large Photometric Surveys
15:30 - 16:00 209 Sara Rezaei Kh. 3D dust distribution in the Galaxy with APOGEE and Gaia; traces of Spiral arms
Wednesday, July 5 10:00 - 11:00 209 Peter Martin Thermal dust emission in intensity and polarization: some quantitative measurements in theoretical context
15:30 - 16:00 209 Anthony Jones Evolutionary dust modelling, theory and observations: What do we really know ?
Thursday, July 6 11:00 - 12:00 209 Bob Benjamin Evidence for Spiral Structure in the Milky Way
15:30 - 16:00 209 Dhanesh Krishnarao Distribution of the Warm Ionized Medium in Spiral Arms
Friday, July 7 10:00 - 11:00 121 Naomi McClure-Griffiths Insights into the evolution of galaxies as traced by hydrogen in the Milky Way and Magellanic Clouds
15:30 - 16:00 209 Karin Sandstrom Interstellar Dust and Molecular Gas at Low Metallicity
16:00 - 17:00 209 Everyone Thunder

Week 2

Date Time Place Speaker Title
Monday, July 10 9:30 209 -- Welcome coffee
10:00 - 11:00 209 Everyone Lightning
13:30 - 14:30 209 Fabian Heitsch Structure Formation in astrophysical gases: a modeler's perspective
15:30 - 16:00 209 Claire Murray Decoding the multi-phase atomic ISM with HI absorption
Tuesday, July 11 10:00 - 11:00 209 Eddie Schlafly Dust and the Extinction Curve in 3D
15:30 - 16:00 209 Kirill Tchernyshyov Detecting spiral structure induced ISM motions with kinetic tomography
Wednesday, July 12 10:00 - 11:00 121 Joao Alves Things we didn't know existed: clouds with power-law PDFs, filaments as pillars, and a physically motivated definition for dense cores
15:30 - 16:00 209 Di Li How to Trace the HI-H2 Transition in the ISM
Thursday, July 13 10:00 - 11:00 209 Tom Troland Magnetic fields in the Galaxy from the diffuse ISM to PDRs to molecular cores – How strong are they and why?
14:30 - 15:30 209 Everyone Thunder
15:30 - 16:00 209 Benoit Commercon The interplay of magnetic fields and radiative feedback on the collapse and fragmentation of prestellar dense cores
Friday, July 14 -- 209 no talk today national holiday

Week 3

Date Time Place Speaker Title
Monday, July 17 9:30 209 -- Welcome coffee
10:00 - 11:00 209 Everyone Lightning
13:30 - 14:30 209 Susan Clark Magnetism and Morphology in the ISM
15:30 - 16:00 209 Gilles Joncas Looking for evolutionary signatures in four high galactic latitude translucent molecular clouds through the HI-CO-dust connection
Tuesday, July 18 10:00 - 11:00 209 Tim Robishaw Measuring B in the ISM
15:30 - 16:00 209 Richard Crutcher Toward Observing the 3D Magnetic Vector in Molecular Clouds
Wednesday, July 19 10:00 - 11:00 209 Mark Heyer Molecular clouds and striations
14:00 - 15:00 121 Norman Murray On the interplay between giant molecular clouds and star formation
Thursday, July 20 10:00 - 11:00 209 Enrique Vazquez-Semadeni Molecular Cloud Formation, Evolution, and Hierarchical Collapse
15:30 - 16:00 209 Gina Panopoulou Do molecular cloud filaments really have a characteristic width?
Friday, July 21 10:00 - 11:00 209 Blakesley Burkhart New Diagnostics of MHD Turbulence in the Multiphase Interstellar Medium
14:30 - 15:30 209 Everyone Thunder
15:30 - 16:00 209 Chang-Goo Kim Three-phase Interstellar medium in Galaxies Resolving Evolution with Star formation and Supernova feedback (TIGRESS)

Week 4

Date Time Place Speaker Title
Monday, July 24 9:30 209 -- Welcome coffee
10:00 - 11:00 209 Everyone Lightning
13:30 - 14:30 209 Patrick Hennebelle From diffuse ISM to molecular cores
15:30 - 16:00 209 Robi Banerjee Star formation out of the magnetised ISM
Tuesday, July 25 10:00 - 11:00 209 Juan Soler Two or three tricks from pattern recognition applied to the study of the interstellar magnetic field
15:30 - 16:00 209 Jean-Francois Robitaille Turbulence, star formation and magnetic field seen through multi-scale analysis techniques
Wednesday, July 26 10:00 - 11:00 209 Alex Hill Stellar feedback, turbulence, and the warm ionized medium
15:30 - 16:00 209 Alex Lazarian Gradient Technique as a new way to trace magnetic field and the ISM physics
Thursday, July 27 10:00 - 11:00 121 Katia Ferriere X-shaped magnetic fields in galactic halos
15:30 - 16:00 209 Vibor Jelic Faraday tomography of the local ISM
Friday, July 28 10:00 - 11:00 209 Eva Ntormousi Closing talk on numerical aspects
14:30 - 15:30 209 Everyone Thunder
15:30 - 16:00 209 Marc-Antoine Miville-Deschenes Closing talk on observational aspects