The daily schedule is composed of two or three informal talks per day, one or two in the morning and one in the afternoon. Each talk is 30min, questions included. The rest of the time is dedicated to discussions and personnal or collaborative work.

Every Monday morning starts with a Lightning session where participants present themselves in 2 minutes maximum, using a single slide. Every Friday afternoon ends with a Thunder session where participants are invited to present work done during the week.

The following schedule is still being updated.

Week 1

Date Time Speaker Topic
Monday, September 16 9:00 -- Welcome coffee
10:00 - 11:00 Everyone Introduction & Lightning
11:00 - 11:30 McClure-Griffiths, Naomi Small-scale effects in Large-scale Outflows
16:00 - 16:30 Pingel, Nickolas The Turbulent HI Properties in the SMC as Revealed by GASKAP
Tuesday, September 17 10:00 - 10:30 Ferrière, Katia Plasma turbulence in the ISM
10:30 - 11:00 Hill, Alex The Stability of the Three-Phase ISM
16:00 - 16:30 Koertgen, Bastian Cloud formation from large to small scales: Global simulations of magnetised disc galaxies
17:30 - 19:00 -- Happy Hour
Wednesday, September 18 10:00 - 10:30 Guillet, Vincent Spectral energy distribution of dust polarized emission in molecular regions, as seen by Planck in the submillimeter
10:30 - 11:00 Green, Gregory Mapping dust in the entire Galactic Plane with deep multiband photometry
16:00 - 16:30 Wu, John Visualizing galaxy structures and ISM properties using deep learning
Thursday, September 19 10:00 - 10:30 Burkhart, Blakesley An Investigation of the Impact of Stellar Feedback on Time-varying Analytic Models of Star Formation
16:00 - 16:30 Wenger, Trey Galactic HII Regions: Morphological and Chemical Structure in the Milky Way
19:00 - -- Dinner
Friday, September 20 11:00 - 11:30 Martin, Peter Some explorations of/with dust in GMCs
16:00 - 17:00 Everyone Thunder

Week 2

Date Time Speaker Title
Monday, September 23 9:00 -- Welcome coffee
10:00 - 11:00 Everyone Introduction & Lightning
11:00 - 11:30 Bontemps, Sylvain Cloud, filament formation with the new generation of FIR instruments
16:00 - 16:30 Ntormousi, Evangelia The magnetized ISM, from molecular clouds to galaxies
Tuesday, September 24 10:00 - 10:30 Clark, Susan The magnetic interstellar medium in three dimensions
10:30 - 11:00 Koch, Eric HI & CO Kinematics in the Local Group
16:00 - 16:30 Krishnarao, Dhanesh The Ionized ISM Around Bars: Using galaxies to Understand The Galaxy
17:30 - 19:00 -- Happy Hour
Wednesday, September 25 10:00 - 10:30 Jameson, Katie Cold Neutral and Molecular Gas in the Small Magellanic Cloud
10:30 - 11:00 Gong, Munan Observing molecular clouds in numerical simulations
14:00 - 15:00 Marchal, Antoine On the multiphase structure of the turbulent interstellar medium - Ph.D defense
Thursday, September 26 10:00 - 10:30 Benjamin, Bob Star Formation and Sources of Ionization in the Inner Milky Way
10:30 - 11:00 Fissel, Laura Magnetic Fields, Molecular Clouds and Star Formation
16:00 - 16:30 Wang, Yuan The distribution of the atomic gas in the northern galactic plane seen by THOR
19:00 - -- Dinner
Friday, September 27 11:00 - 11:30 Peek, Josh Can you believe your eyes?
16:00 - 17:00 Everyone Thunder

Week 3

Date Time Speaker Title
Monday, September 30 9:00 -- Welcome coffee
10:00 - 11:00 Everyone Introduction & Lightning
11:00 - 11:30 Ballesteros-Paredes, Javier Whats the physics behind the Larson's relations
16:00 - 16:30 Kim, Jeong-Gyu Modeling UV Radiation Feedback from Massive Stars
Tuesday, October 1st 10:00 - 10:30 Alves, João A Galactic-scale gas wave in the Solar Neighborhood
10:30 - 11:00 Frédérique Motte What if stars would inherit their properties from those of their parental cloud/filament?
16:00 - 16:30 Evans, Neal The Central Problem of Star Formation: Why So Slow?
17:30 - 19:00 -- Happy Hour
Wednesday, October 2nd 10:00 - 10:30 Dickey, John Using Faraday Synthesis to link the B field on large and small scales
10:30 - 11:00 Joncas, Gilles A go at the thermodynamics of HII regions: the case of Sh2-158
16:00 - 16:30 Goodman, Alyssa The Path to Newton
Thursday, October 3rd 10:00 - 10:30 Soler, Juan Diego Understanding the structure of the magnetized interstellar medium using circular statistics.
10:30 - 11:00 Tahani, Mehrnoosh The large-scale structure of magnetic fields associated with filamentary molecular clouds
16:00 - 16:30 Vazquez-Semadeni, Enrique From filaments to clusters through Global Hierarchical Collapse
19:00 - -- Dinner
Friday, October 4th 10:00 - 10:30 Camacho, Vianey From a low-mass cloud to an active star forming region
10:30 - 11:00 Silsbee, Kedron Cosmic Rays in Molecular Clouds: Transport Models and Observational Constraints
16:00 - 17:00 Everyone Thunder

Week 4

Date Time Speaker Title
Monday, October 7 9:00 -- Welcome coffee
10:00 - 11:00 Everyone Introduction & Lightning
11:00 - 11:30 Shu-ichiro Inutsuka Filament Paradigm and A Unified Picture of Star Formation in the Galactic Disk
16:00 - 16:30 Zucker, Catherine Mapping our Local Milky Way: Dust, Gas (& Stars)
Tuesday, October 8 10:00 - 10:30 Lazarian, Alex
10:30 - 11:00 Pellegrini, Eric Understanding Stellar Feedback and the ISM through SDSS-V LVM and Population Synthesis of Clouds
16:00 - 16:30 André, Philippe The role of molecular filaments in the origin of the prestellar core mass function and stellar initial mass function
17:30 - 19:00 -- Happy Hour
Wednesday, October 9 10:00 - 10:30 Heyer, Mark Assembly of giant molecular clouds in the Milky Way
10:30 - 11:00 Dawson, Joanne OH What a (Flipping) Lovely Molecule: Tracing ISM physics with the OH Satellite Line "Flip"
16:00 - 16:30 Joubaud, Theo Gas shells and magnetic fields in the Orion-Eridanus superbubble
Thursday, October 10 10:00 - 10:30 Heitsch, Fabian Gas Dynamics and Star Formation near Black Holes
10:30 - 11:00 Miville-Deschenes, Marc-Antoine The multi-phase nature of the interstellar medium
16:00 - 16:30 Hennebelle, Patrick
19:00 - Dinner
Friday, October 11 11:00 - 11:30 Dashyan, Gohar Cosmic ray feedback from supernovae in dwarf galaxies
16:00 - 17:00 Everyone Thunder