Ramses User meeting 2018 - Sciencesconf.org

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