Ramses User Meeting 2018

17-21 Sep 2018 Lyon (France)

Program

Week Mon. 17 Tue. 18 Wed. 19 Thu. 20 Fri. 21 List

	Mon. 17	Tue. 18	Wed. 19	Thu. 20	Fri. 21
09:00 10:00 11:00 12:00 13:00 14:00 15:00 16:00 17:00 18:00 19:00 20:00 21:00	Star formation Black holes 10:30 - 12:10 (1h40) Star formation Salle de conférence de la MILC Benoit Commercon › Prospects in modeling low-mass star formation - Michael Küffmeier, Niels Bohr Institute 10:30-10:50 (20min) › The Hall effect in RAMSES for star formation - Pierre Marchand, Osaka University 10:50-11:10 (20min) › Dust dynamics on adaptative mesh-refinement grids in the diffusion approximation - Ugo Lebreuilly, Centre de Recherche Astrophysique de Lyon 11:10-11:30 (20min) › Hybrid Radiative Transfer Methods for Prestellar Isolated Core Collapse : A comparison of RT methods for Massive Star Formation - Raphaël Mignon-Risse, Université Paris Diderot - Paris 7 11:30-11:50 (20min) 11:50 - 12:10 (20min) Black holes Salle de conférence de la MILC Benoit Commercon › Growing black holes in high-redshift galaxies during the Epoch of Reionization - Maxime Trebitsch, Institut d'Astrophysique de Paris (IAP) 11:50-12:10 (20min) Lunch 12:10 - 14:00 (1h50) Lunch Black holes Computational astrophysics 14:00 - 15:00 (1h) Black holes Salle de conférence de la MILC Adrianne Slyz › Supermassive black hole dynamics under the grid - Hugo Pfister, Institut d'Astrophysique de Paris 14:00-14:20 (20min) 14:20 - 15:00 (40min) Computational astrophysics Salle de conférence de la MILC Adrianne Slyz › HERCULE data management library : boosting RAMSES I/O for exascale era - Loic Strafella, Institut de Recherches sur les lois Fondamentales de l'Univers 14:20-14:40 (20min) › Glnemo2, an interactive 3D visualization program for N-body data - Jean-Charles Lambert, Laboratoire d'Astrophysique de Marseille, Laboratoire d'Astrophysique de Marseille 14:40-15:00 (20min) Coffee break 15:00 - 15:30 (30min) Coffee break Salle de conférence de la MILC Computational astrophysics The ISM and feedback 15:30 - 16:30 (1h) Computational astrophysics Adrianne Slyz › MacLeCool: A Machine Learning Cooling Emulator for RAMSES - Julien Devriendt, Oxford University 15:30-15:50 (20min) › Cosmic ray physics in Ramses - Yohan Dubois, Institut d'Astrophysique de Paris 15:50-16:10 (20min) 16:10 - 16:30 (20min) The ISM and feedback Salle de conférence de la MILC Adrianne Slyz › The effect of cosmic rays on momentum injection, wind driving and star formation - Gohar Dashyan, IAP 16:10-16:30 (20min)	The ISM and feedback 9:00 - 10:20 (1h20) The ISM and feedback Salle de conférence de la MILC Julien Devriendt › 1. Hierarchical Scales of Clump Clusters in High-Redshift Disk Galaxies / 2. MERA: A RAMSES Post Processing Tool Written in The Julia Language - Behrendt Manuel, MPI for extraterrestrial Physics 09:00-09:20 (20min) › Globular cluster ISM: how to get rid of it? - william chantereau, Astrophysics Research Institute [Liverpool] 09:20-09:40 (20min) › The addition of molecular hydrogen to RAMSES-RT - Sarah Nickerson, University of Zurich 09:40-10:00 (20min) › Lyman radiation hydrodynamics in turbulent star-forming gas clouds in galaxies - Koki Kakiichi, University College, London 10:00-10:20 (20min) Coffee break 10:20 - 10:50 (30min) Coffee break Salle de conférence de la MILC The ISM and feedback 10:50 - 12:10 (1h20) The ISM and feedback Salle de conférence de la MILC Julien Devriendt › Numerical simulations of photoevaporating molecular clumps - Davide Decataldo, Scuola Normale Superiore di Pisa 10:50-11:10 (20min) › Feedback in Molecular Clouds - Geen Sam, ITA/ZAH University of Heidelberg 11:10-11:30 (20min) › Impact of strong Lyman alpha pressure on metal-poor dwarf galaxies - Taysun Kimm, Yonsei University 11:30-11:50 (20min) › Interacting stellar winds: clump formation and accretion onto SGR A* - Diego Calderón, Max-Planck-Institut für extraterrestrische Physik, Pontificia Universidad Católica de Chile 11:50-12:10 (20min) Lunch 12:10 - 14:00 (1h50) Lunch Galaxy clusters 14:00 - 15:00 (1h) Galaxy clusters Salle de conférence de la MILC Sugata Kaviraj › New Cluster simulation with NewHorizon resolution - Sukyoung Yi, Yonsei University 14:00-14:20 (20min) › YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters - San Han, Yonsei University 14:20-14:40 (20min) › Simulating objects of the local Universe: the Virgo cluster of galaxies, a case study - Jenny Sorce, CRAL 14:40-15:00 (20min) Coffee break 15:00 - 15:30 (30min) Coffee break Salle de conférence de la MILC Galaxy clusters Galaxy formation 15:30 - 16:30 (1h) Galaxy clusters Salle de conférence de la MILC Sugata Kaviraj › Revealing the quenching history of cluster galaxies using Phase-space Analysis - Jinsu Rhee, Yonsei University 15:30-15:50 (20min) 15:50 - 16:30 (40min) Galaxy formation Salle de conférence de la MILC Sugata Kaviraj › What are the properties of kpc scale filaments at high redshift? - Marius Ramsoy, University of Oxford [Oxford] 15:50-16:10 (20min) › Horizon Run 5 - A very large volume hydrodynamical simulation - Owain Snaith, KIAS 16:10-16:30 (20min) Wine and cheese at Lyon Observatory 17:00 - 21:00 (4h) Wine and cheese at Lyon Observatory	Galaxy formation 9:00 - 10:20 (1h20) Galaxy formation Salle de conférence de la MILC Oliver Hahn › cosmICweb: An online database for cosmological initial conditions for zoom-in simulations - Michael Buehlmann, Observatoire de la Côte dÁzur 09:00-09:20 (20min) › The development of massive field galaxies in the first half of the cosmic history - Minjung Park, Yonsei Univ 09:20-09:40 (20min) › Why do massive disc galaxies exist? - Sugata Kaviraj, University of Hertfordshire [Hatfield] 09:40-10:00 (20min) › Predictions for the low surface-brightness Universe from the Horizon-AGN simulation - Garreth Martin, University of Hertfordshire 10:00-10:20 (20min) Coffee break 10:20 - 10:50 (30min) Coffee break Salle de conférence de la MILC Galaxy formation 10:50 - 12:10 (1h20) Galaxy formation Salle de conférence de la MILC Oliver Hahn › Forming spheroids in single minor mergers - Ryan Jackson, University of Hertfordshire 10:50-11:10 (20min) › Gas fraction of galaxies and impact of mergers across cosmic times - Jeremy Fensch, European Southern Observatory 11:10-11:30 (20min) › The origin of galactic magnetic fields - Sergio Martin-Alvarez, University of Oxford [Oxford] 11:30-11:50 (20min) › Cosmological zoom-in Milky-way like galaxies: trying different baryonic physics schemes - Arturo Nuñez-Castiñeyra, Laboratoire d'Astrophysique de Marseille 11:50-12:10 (20min) Lunch 12:10 - 14:00 (1h50) Lunch Galaxy formation 14:00 - 15:00 (1h) Galaxy formation Salle de conférence de la MILC Yohan Dubois › A zoomed view of galaxies at high redshift. - Andrea Pallottini, Centro Fermi, Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi" Piazza del Viminale 1 Roma, 00184, Italy 14:00-14:20 (20min) › Why are my Lya spectra weird looking? - Jérémy Blaizot, Centre de Recherche Astrophysique de Lyon 14:20-14:40 (20min) › The photon budget of galaxies during the epoch of reionisation in the Cosmic Dawn II simulation - Joseph Lewis, Observatoire astronomique de Strasbourg 14:40-15:00 (20min) Coffee break 15:00 - 15:30 (30min) Coffee break Salle de conférence de la MILC Computational astrophysics 15:30 - 16:00 (30min) Computational astrophysics Salle de conférence de la MILC Yohan Dubois › RAMSES-NG and the future - Romain Teyssier, ICS Zürich 15:30-16:00 (30min) Discussion and hackathon plan 16:00 - 17:00 (1h) Discussion and hackathon plan Salle de conférence de la MILC	Hackathon 9:00 - 17:00 (8h) Hackathon École Normale Supérieure de Lyon	Hackathon 9:00 - 17:00 (8h) Hackathon École Normale Supérieure de Lyon

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