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