Ramses User Meeting 2021
27-29 Sep 2021
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Program
Week
Mon. 27
Tue. 28
Wed. 29
List
Mon. 27
Tue. 28
Wed. 29
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
Welcome
9:15 - 9:30 (15min)
Welcome
The LOC
Galaxy clusters / black holes
9:30 - 10:50 (1h20)
Galaxy clusters / black holes
Adrianne Slyz
›
Super-Eddington in a collapsing DM halo at high-z
- Warren Massonneau, Institut d'Astrophysique de Paris
09:30-09:50 (20min)
›
YZiCS: On the Mass Segregation of Galaxies in Clusters
- Seonwoo Kim, Yonsei University
09:50-10:10 (20min)
›
Cosmic rays and the multi-phase gas in clusters
- Ricarda Beckmann, Institute of Astronomy, University of Cambridge
10:10-10:30 (20min)
›
Tidal Disruption Events under the grid
- Hugo Pfister, The University of Hong Kong
10:30-10:50 (20min)
Coffee break
10:50 - 11:10 (20min)
Coffee break
Black holes / the ISM
11:10 - 12:30 (1h20)
Black holes / the ISM
Adrianne Slyz
›
Feedback from Active Galactic Nuclei in Galaxy Groups and Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground between Clusters and Galaxies
- Amandine Le Brun, Laboratoire Univers et Théories, Université PSL, Département d'Astrophysique (DAp)
11:10-11:30 (20min)
›
Dynamics of massive black holes in cosmological simulations
- Marta Volonteri, Institut d'Astrophysique de Paris
11:30-11:50 (20min)
›
PRALINES: LyC and LyA escape from GMCs
- Taysun Kimm, Yonsei University
11:50-12:10 (20min)
›
Revisiting Stellar Winds: What do they do, and what does this mean for RAMSES simulations?
- Geen Sam, University of Amsterdam [Amsterdam]
12:10-12:30 (20min)
Lunch
12:30 - 14:00 (1h30)
Lunch
The ISM / star and planet formation
14:00 - 15:20 (1h20)
The ISM / star and planet formation
Ricarda Beckmann
›
Explaining the Schmidt-Kennicutt law: the crucial role of large-scale turbulent driving
- Noé Brucy, Astrophysique Interprétation Modélisation
14:00-14:20 (20min)
›
Second generation star formation in globular clusters of different masses
- Asiyeh Yaghoobi, Department of Physics, Institute for Advanced Studies in Basic Sciences (IASBS), 444 Prof. Yousef Sobouti Blvd., 45137-66731, Zanjan, Iran
14:20-14:40 (20min)
›
The role of Type Ia supernova feedback on the second generation formation in globular clusters
- Elena Lacchin, INAF – OAS, Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Department of Physics and Astronomy, University of Bologna
14:40-15:00 (20min)
›
Protoplanetary disks population formation in massive clumps.
- Ugo Lebreuilly, CEA Saclay
15:00-15:20 (20min)
Coffee break
15:20 - 15:40 (20min)
Coffee break
Star and planet formation / computational methods
15:40 - 17:00 (1h20)
Star and planet formation / computational methods
Ricarda Beckmann
›
Massive star formation: a tale of accretion, ejection and multiplicity
- Raphaël Mignon-Risse, AstroParticule & Cosmologie
15:40-16:00 (20min)
›
Modelling the Biermann battery in the RAMSES code
- Omar Attia, University of Geneva
16:00-16:20 (20min)
›
Stellar magneto-convection with RAMSES
- José Roberto Canivete Cuissa, Institute of Computational Science
16:20-16:40 (20min)
›
Fast methods for tracking grain coagulation and ionization
- Pierre Marchand, American Museum of Natural History
16:40-17:00 (20min)
Computational methods
9:30 - 10:50 (1h20)
Computational methods
Clotilde Laigle
›
New Ramses simulation projects at Yonsei
- Sukyoung Yi, Yonsei University
09:30-09:50 (20min)
›
Galaxy Identification with the 6D Friends-of-friend Algorithm on the NewHorizon Simulation and its Comparison to the GALAXYMaker Data
- Jinsu Rhee, Yonsei University
09:50-10:10 (20min)
›
Dust in Ramses galaxies with more than ad hoc dust-to-metal ratios
- Yohan Dubois, Institut d'Astrophysique de Paris
10:10-10:30 (20min)
›
LightAMR standardized data structure and associated lossless compression algorithms: RAMSES datasets use cases.
- Loic Strafella, Institut de Recherches sur les lois Fondamentales de lÚnivers
10:30-10:50 (20min)
Coffee break
10:50 - 11:10 (20min)
Coffee break
Computational methods / the EoR
11:10 - 12:30 (1h20)
Computational methods / the EoR
Clotilde Laigle
›
Bi-Poisson: a RAMSES implementation of two coupled Poisson equations
- Clément Stahl, AstroParticule et Cosmologie
11:10-11:30 (20min)
›
The Great Merge: progress towards a unified RAMSES
- Tine Colman, CEA- Saclay
11:30-11:50 (20min)
›
The clumping factor of the IGM at the epoch of reionization in the SPHINX simulations
- Taehwa Yoo, Yonsei University
11:50-12:10 (20min)
›
Cosmic Dawn III: the latest and largest radiation-hydrodynamical simulation of the Epoch of Reionization
- Pierre Ocvirk, Observatoire de Strasbourg
12:10-12:30 (20min)
Lunch
12:30 - 14:00 (1h30)
Lunch
The EoR / galaxy formation
14:00 - 15:20 (1h20)
The EoR / galaxy formation
Amandine Le Brun
›
Reproducing the latest determinations of the mean free path of ionising photons in CoDa III
- Joe Lewis, University of Heidelberg
14:00-14:20 (20min)
›
Radiation-coupled Primordial Chemistry in Simulations of the First Galaxies
- Sean Barrett, Sub-department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
14:20-14:40 (20min)
›
Baryon drift effects at high redshift
-
14:40-15:00 (20min)
›
Star formation in high-redshift clumpy galaxies
- Jeremy Fensch, CRAL
15:00-15:20 (20min)
Coffee break
15:20 - 15:40 (20min)
Coffee break
Galaxy formation
15:40 - 17:00 (1h20)
Galaxy formation
Amandine Le Brun
›
The formation of dark-matter-deficient dwarf galaxies
- Ryan Jackson, University of Hertfordshire
15:40-16:00 (20min)
›
The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
- Martin Rey, Oxford Astrophysics, Lund Observatory
16:00-16:20 (20min)
›
Star Clusters and Galaxies within EDGE
- Ethan Taylor, University of Surrey
16:20-16:40 (20min)
›
The Galactic dynamo
- Romain Teyssier, Princeton University
16:40-17:00 (20min)
Galaxy formation
9:30 - 10:50 (1h20)
Galaxy formation
Oscar Agertz
›
The star formation quenching and transition epoch in Horizon-AGN galaxies
- Seyoung Jeon, Yonsei University
09:30-09:50 (20min)
›
NewHorizon: the galaxy structure decomposition - photometry vs. kinematics
- Jaekyoung Jang, Yonsei University
09:50-10:10 (20min)
›
Velocity dispersion profiles of NewHorizon galaxies
- San Han, Yonsei University
10:10-10:30 (20min)
›
Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
- Jaehyun Lee, Korea Institute of Advanced Study
10:30-10:50 (20min)
Coffee break
10:50 - 11:10 (20min)
Coffee break
Galaxy formation / computational methods
11:10 - 12:30 (1h20)
Galaxy formation / computational methods
Oscar Agertz
›
The Mochima simulations: testing the effects of baryonic physics on one zoom-in spiral galaxy.
- arturo nuñez-castiñeyra, Laboratoire d'Astrophysique de Marseille
11:10-11:30 (20min)
›
The CGM as a constraint for star formation and feedback subgrid models.
- Maxime Rey, Centre de Recherche Astrophysique de Lyon
11:30-11:50 (20min)
›
The role of cosmic ray feedback in the evolution of galaxies
- Marion Farcy, Centre de Recherche Astrophysique de Lyon
11:50-12:10 (20min)
›
Dyablo : A new hardware-agnostic AMR code for the Ramses community
- Arnaud Durocher, Institut de Recherches sur les lois Fondamentales de l'Univers
12:10-12:30 (20min)
Lunch
12:30 - 14:00 (1h30)
Lunch
Galaxy formation
14:00 - 15:20 (1h20)
Galaxy formation
Sam Geen
›
Dwarf galaxy formation beyond supernovae: magnetism, radiation and cosmic rays
- Sergio Martin-Alvarez, University of Cambridge [Cambridge]
14:00-14:20 (20min)
›
Cosmic rays, explosions and galaxy formation: the deposition of momentum in the ISM and their influence in star formation
-
14:20-14:40 (20min)
›
The causal origin of angular momentum in galaxies
-
14:40-15:00 (20min)
›
The history of the Milky Way told by its mergers
-
15:00-15:20 (20min)
Coffee break
15:20 - 15:40 (20min)
Coffee break
Galaxy formation
15:40 - 16:40 (1h)
Galaxy formation
Sam Geen
›
Cosmic evolution of star formation modes in the Milky Way.
-
15:40-16:00 (20min)
›
Ramses simulations with resolved stars
-
16:00-16:20 (20min)
›
BHs and AGN in 6 large-scale cosmological simulations
- Melanie Habouzit, Max-Planck-Institut für Astronomie
16:20-16:40 (20min)
Wrap-up
16:40 - 16:50 (10min)
Wrap-up
The LOC
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