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Monday, December 11, 2023
| Time | Event | (+) |
| 09:00 - 10:00 | Coffee break (Hall) | |
| 10:00 - 12:10 | Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Joop Schaye | (+) |
| 10:00 - 10:10 | › Welcome - Yohan Dubois, IAP | |
| 10:10 - 10:50 | › Simulating populations of galaxies and their details from the end of the Reionization to the current epoch - Annalisa Pillepich, Max Planck Society (GERMANY) | |
| 10:50 - 11:10 | › Calibrating subgrid feedback in cosmological simulations that include a cold interstellar gas phase - Evgenii Chaikin, Leiden Observatory, Leiden University | |
| 11:10 - 11:30 | › On the universality of star formation efficiency across time - Alvaro Segovia Otero, Lund Observatory | |
| 11:30 - 11:50 | › The interplay of magnetism, radiation and cosmic rays in dwarf galaxy formation - Sergio Martin-Alvarez, Kavli Institute for Particle Astrophysics and Cosmology | |
| 11:50 - 12:10 | › Introducing the NewCluster simulation - Sukyoung Yi, Yonsei University | |
| 12:10 - 13:40 | Lunch | |
| 13:40 - 15:40 | Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Annalisa Pillepich | (+) |
| 13:40 - 14:00 | › Revisiting the Missing Satellite Problem and Starless Subhalos - Seyoung Jeon, Yonsei University | |
| 14:00 - 14:20 | › On the origin of star formation quenching of galaxies in group environments using NewHorizon - Jinsu Rhee, Korea Astronomy and Space science Institute | |
| 14:20 - 14:40 | › Why does the absence of mergers mater? - Florent Renaud, Strasbourg Observatory | |
| 14:40 - 15:00 | › The surprisingly rapid emergence of strong bars in primordial star-forming galaxies - Frédéric Bournaud, AIM/CEA Paris-Saclay | |
| 15:00 - 15:20 | › Star formation across main sequence and quenched galactic environments - Sarah Jeffreson, Harvard-Smithsonian Center for Astrophysics | |
| 15:20 - 15:40 | › Molecular gas in low metallicity galaxies and its implications for star formation - Ava Polzin, University of Chicago | |
| 15:40 - 16:25 | Coffee break (Hall & Entresol) | |
| 16:25 - 18:05 | Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Annalisa Pillepich | (+) |
| 16:25 - 16:45 | › Universality of gravitation-driven isothermal turbulence in galactic disks - Jeremy Fensch, CRAL | |
| 16:45 - 17:05 | › Emergence and cosmic evolution of the Kennicutt-Schmidt relation driven by interstellar turbulence - Katarina Kraljic, Observatoire astronomique de Strasbourg | |
| 17:05 - 17:25 | › The GigaEris Simulation: probing the evolution of disc galaxies evolution at Redshift > 4 - Floor Van Donkelaar, Institute for Computational Science, University of Zurich | |
| 17:25 - 17:45 | › Morphology of High-Redshift Galaxies in the Horizon Run 5 Simulation and JWST Observation - Changbom Park, Korea Institute for Advanced Study | |
| 17:45 - 18:05 | › Three Eras of Computational Cosmology - August Evrard, University of Michigan | |
| 18:05 - 21:00 | Cocktail (Hall & Entresol) |
Tuesday, December 12, 2023
| Time | Event | (+) |
| 09:00 - 10:40 | Galaxies in the first Gyr (Amphitheatre) - Stefanie Walch | (+) |
| 09:00 - 09:40 | › Galaxies in the first Gyr: Frontiers of both theory and observation - Harley Katz, University of Oxford | |
| 09:40 - 10:00 | › Early Galaxy Formation and Cosmic Reionization in the JWST Era - Hakim Atek, Institut d'Astrophysique de Paris | |
| 10:00 - 10:20 | › Pitfalls of numerical simulations in the JWST era. - Andrea Pallottini, Scuola Normale Superiore | |
| 10:20 - 10:40 | › New Simulations of Feedback-Free Starbursts at Cosmic Dawn - Avishai Dekel, The Hebrew University of Jerusalem | |
| 10:40 - 11:10 | Coffee break (Hall & Entresol) | |
| 11:10 - 12:30 | Galaxies in the first Gyr (Amphitheatre) - Stefanie Walch | (+) |
| 11:10 - 11:30 | › Bursty star formation in galaxies at cosmic dawn from cosmological zoom-in simulations - Guochao Sun, Northwestern University | |
| 11:30 - 11:50 | › Simulating Cosmic Reionization on all scales - Ilian Iliev, Astronomy Centre, University of Sussex | |
| 11:50 - 12:10 | › Dusty galaxies powering Reionization in Cosmic Dawn III - Joseph Lewis, Universität Heidelberg, Max Planck Institute for Astronomy | |
| 12:10 - 12:30 | › SPICE : Connecting the effect of stellar feedback in first galaxies and cosmic reionisation - Aniket Bhagwat, Max-Planck-Institut für Astrophysik | |
| 12:30 - 14:00 | Lunch | |
| 14:00 - 15:40 | Are cosmic rays a missing ingredient? (Amphitheatre) - Thorsten Naab | (+) |
| 14:00 - 14:40 | › Cosmic Ray Feedback from Supernovae to Galaxy Clusters - Mateusz Ruszkowski, Department of Astronomy, University of Michigan-Ann Arbor | |
| 14:40 - 15:00 | › Cosmic-ray diffusion and the multi-phase interstellar medium in a dwarf galaxy. I. Large-scale properties and γ-ray luminosities - Arturo Nuñez-Castiñeyra, CEA- Saclay | |
| 15:00 - 15:20 | › A multi-frequency view on simulating galaxy formation with cosmic rays - Maria Werhahn, Max Planck Institute for Astrophysics | |
| 15:20 - 15:40 | › Cosmic ray feedback and magnetic dynamos in galaxies - Christoph Pfrommer, Leibniz Institute for Astrophysics Potsdam | |
| 15:40 - 16:25 | Coffee break (Hall & Entresol) | |
| 16:25 - 17:05 | Are cosmic rays a missing ingredient? (Amphitheatre) - Thorsten Naab | (+) |
| 16:25 - 16:45 | › Comic ray-supported Galactic Outflows: Probing kinematics and multiphase gas strucutre within ISM simulations - Tim-Eric Rathjen, University of Cologne | |
| 16:45 - 17:05 | › The impact of cosmic rays on the outflow production and composition - Nicolas Peschken, Galileo Galilei Institute for Theoretical Physics | |
| 17:05 - 18:05 | Can we make robust predictions about dust? (Amphitheatre) - Thorsten Naab | (+) |
| 17:05 - 17:25 | › Dusty, star-forming galaxies at z=2: Can simulations reproduce these extreme galaxies? - Andrea Gebek, Universiteit Gent = Ghent University | |
| 17:25 - 17:45 | › Modelling early massive dusty galaxies and their properties with the Obelisk simulation - Maxime Trebitsch, Kapteyn Astronomical Institute |
Wednesday, December 13, 2023
| Time | Event | (+) |
| 09:00 - 10:40 | Galaxies in non-standard cosmologies (Amphitheatre) - Volker Springel | (+) |
| 09:00 - 09:40 | › Galaxy formation in non-standard cosmological models - Baojiu Li, Durham University | |
| 09:40 - 10:00 | › The impact of Baryons vs. Self-Interacting Dark Matter on Galaxy Formation - Camila Correa, CEA Paris-Saclay | |
| 10:00 - 10:20 | › Galaxy formation and primordial non-Gaussianities - Clément Stahl, Observatoire astronomique de Strasbourg | |
| 10:20 - 10:40 | Large-scale structures and galaxies (Amphitheatre) - Volker Springel | (+) |
| 10:20 - 10:40 | › Towards constraining the gas properties in the cosmic web - Yan-Chuan Cai, Institute for Astronomy, University of Edinburgh | |
| 10:40 - 11:10 | Coffee break (Hall & Entresol) | |
| 11:10 - 12:30 | Large-scale structures and galaxies (Amphitheatre) - Volker Springel | (+) |
| 11:10 - 11:30 | › Constraints on particle dark matter using the Intergalactic Medium - Matteo VIEL, Scuola Internazionale Superiore di Studi Avanzati / International School for Advanced Studies | |
| 11:30 - 11:50 | › the cosmic web - CGM interface from Milky Ways to Clusters - Charlotte Welker, City University of New York | |
| 11:50 - 12:10 | › Flows around galaxies: I. The dependence of galaxy connectivity on cosmic environments and effects on the star formation rate - Daniela Galárraga-Espinosa, Max Planck Institute for Astrophysics | |
| 12:10 - 12:30 | › On the causal origin of dark matter halo and galaxy angular momentum: replacing galaxies in their cosmological context - Corentin Cadiou, Division of Astrophysics, Department of Physics [Lund University], IAP | |
| 12:30 - 14:00 | Lunch | |
| 14:00 - 18:00 | Nick Kaiser Tribute (Amphitheatre) | |
| 18:00 - 20:00 | Cocktail (Hall & Forum) | |
| 20:00 - 23:00 | Conference Dinner (Madame Brasserie - Tour Eiffel) |
Thursday, December 14, 2023
| Time | Event | (+) |
| 09:40 - 11:00 | Large-scale structures and galaxies (Amphitheatre) - Harley Katz | (+) |
| 09:40 - 10:20 | › Simulations at the interface between large-scale structure and galaxy formation - Joop Schaye, Leiden Observatory, Leiden University | |
| 10:20 - 10:40 | › The FLAMINGO suite of cosmological simulations - Schaller Matthieu, Lorentz Institute | |
| 10:40 - 11:00 | › Galaxy groups and clusters in FLAMINGO - Joey Braspenning, Leiden Observatory | |
| 11:00 - 11:30 | Coffee break (Hall & Entresol) | |
| 11:30 - 12:30 | The nature of the circum-galactic medium (Amphitheatre) - Harley Katz | (+) |
| 11:30 - 12:10 | › The multi-scale multi-phase Circum-Galactic Medium - Celine Peroux, European Southern Observatory | |
| 12:10 - 12:30 | › Resolving the physics of multi-scale gaseous halos - Dylan Nelson, Heidelberg University | |
| 12:30 - 14:00 | Lunch | |
| 14:00 - 15:40 | The nature of the circum-galactic medium (Amphitheatre) - Sukyoung Yi | (+) |
| 14:00 - 14:20 | › Constraining feedback processes with the circum-galactic medium - Maxime Rey, Yonsei University | |
| 14:20 - 15:00 | › Arkenstone: A Multi-Scale Approach to Galaxy Formation - Drummond Fielding, Center for Computational Astrophysics, Flatiron Institute | |
| 15:00 - 15:20 | › Unraveling Multiphase Dynamics: Stirring the Magnetic spaghetti in a Turbulent sauce - Hitesh Kishore Das, Max Planck Institute for Astrophysics | |
| 15:20 - 15:40 | › The origin of multiphase galactic outflows - Ulrich Steinwandel, Center for Computational Astrophysics (CCA, Simons Foundation) | |
| 15:40 - 16:25 | Coffee break (Hall & Entresol) | |
| 16:25 - 17:05 | The nature of the circum-galactic medium (Amphitheatre) - Sukyoung Yi | (+) |
| 16:25 - 16:45 | › Confronting Lyman alpha profiles of high-z galaxies with simulations with strong stellar feedback - Taysun Kimm, Yonsei University | |
| 16:45 - 17:05 | › Constraining the flows of gas around galaxies with Lyman-alpha observations -- insights from simulations - Jeremy Blaizot, Centre de Recherche Astrophysique de Lyon | |
| 17:05 - 18:05 | Feedback from active galactic nuclei (Amphitheatre) - Sukyoung Yi | (+) |
| 17:05 - 17:25 | › The kinematics and observable properties of AGN jets and cavities with cosmological simulations - Laura Di Federico, Universitäts-Sternwarte München, Ludwig-Maximilians-Universität | |
| 17:25 - 17:45 | › The Significance of Recycled Gas: The Primary Fuel for SMBH Accretion in Cosmological Simulations - Ena Choi, University of Seoul | |
| 17:45 - 18:05 | › Multimessenger study of merging massive black holes in the Obelisk simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations - Chi An Dong Páez, Institut d'Astrophysique de Paris |
Friday, December 15, 2023
| Time | Event | (+) |
| 09:00 - 10:40 | Feedback from active galactic nuclei (Amphitheatre) - Marta Volonteri | (+) |
| 09:00 - 09:40 | › Feedback from AGN: Physics & Numerics - Tiago Costa, Newcastle University | |
| 09:40 - 10:00 | › GRMHD Simulations Meet Galactic Evolution: A Refined Model for AGN Feedback - Ivan Almeida, Newcastle University [Newcastle], Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] | |
| 10:00 - 10:20 | › New hyper-refinement simulations for long-standing problems in black hole-galaxy coevolution - Daniel Angles-Alcazar, University of Connecticut | |
| 10:20 - 10:40 | › Super-Eddington accretion during early black hole growth - Brian Jiang, University of Cambridge [UK] | |
| 10:40 - 11:10 | Coffee break (Hall & Entresol) | |
| 11:10 - 12:30 | Feedback from active galactic nuclei (Amphitheatre) - Marta Volonteri | (+) |
| 11:10 - 11:30 | › Settling SMBH at the center of galaxies in the simulation - San Han, Yonsei University | |
| 11:30 - 11:50 | › High-performance galaxy formation simulations with accurate massive black hole dynamics - Antti Rantala, Max Planck Institute for Astrophysics | |
| 11:50 - 12:10 | › Intermediate mass black hole feedback in dwarf galaxy simulations with a resolved ISM and accurate nuclear stellar dynamics - Christian Partmann, Max-Planck-Institut für Astrophysik | |
| 12:10 - 12:30 | › AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows? - Samuel Ward, European Southern Observatory, Newcastle University | |
| 12:30 - 14:00 | Lunch (Amphitheatre) | |
| 14:00 - 15:20 | Feedback from stars (Amphitheatre) - Romain Teyssier | (+) |
| 14:00 - 14:40 | › Feedback from stars - Thorsten Naab, Max Planck Institute for Astrophysics | |
| 14:40 - 15:00 | › Multi-phase gas in cosmological galaxy formation simulations - Rainer Weinberger, Leibniz Institute for Astrophysics Potsdam | |
| 15:00 - 15:20 | › Simulating the formation of globular clusters and their multiple populations in low-metallicity dwarf galaxies - Natalia Lahén, Max Planck Institute for Astrophysics | |
| 15:20 - 15:50 | Coffee break (Hall & Entresol) | |
| 15:50 - 17:10 | Feedback from stars (Amphitheatre) - Romain Teyssier | (+) |
| 15:50 - 16:30 | › The exciting (and uncertain) world of modeling dust in galaxy simulations - Desika Narayanan, University of Florida | |
| 16:30 - 16:50 | › Radiation-hydrodynamic simulations of dwarf galaxies with metallicity dependent feedback from individual stars - Yunwei Deng, Department of Astronomy, Tsinghua University | |
| 16:50 - 17:10 | › Resolved AGN disks in cosmological zoom simulations - Norman Murray, Canadian Institute for Theoretical Astrophysics (CITA), University of Toronto |
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