Important dates
Monday – 20 July
8:15 – 9:00
Welcome Coffee & Registration
9:00 – 9:10
Opening Remarks
Norbert Werner | Masaryk University
9:10 – 9:35
Recent updates on ICM turbulence
Irina Zhuravleva | U Chicago
9:35 – 10:00
Probing ICM Turbulence with XRISM: Comparisons with Cosmological Simulations
Nhut Truong | NASA GSFC/UMD
10:00 – 10:25
ICM Yesterday, Today and Tomorrow: turbulence, multi-phase cellularisation, nonthermal equilibria, and all that
Alex Schekochihin | University of Oxford
10:25 – 11:10
Coffee Break
11:10 – 11:35
Galaxy motion and Gas Dynamics in Cooling Cluster Centres
Brian McNamara | Waterloo Centre for Astrophysics, University of Waterloo
11:35 – 12:00
Rotation, Inflows, Outflows, and Turbulence in Hot Atmospheres from Galaxies to Galaxy Clusters
John ZuHone | Center for Astrophysics | Harvard & Smithsonian
12:00 – 12:25
The role of active galactic nucleus (AGN) jet feedback and cosmological assembly on cool-core cluster entropy and turbulence
Rainer Weinberger | Leibniz-Institute for Astrophysics Potsdam (AIP)
12:25 – 12:40
Posters
12:40 – 14:00
Lunch
14:00 – 14:25
XRISM observations and simulations of the Perseus Cluster (tentative)
Congyao Zhang | Masaryk University
14:25 – 14:50
Disentangling AGN Feedback and Sloshing in the Perseus Cluster with XRISM: Insights from Idealized Simulations
Elena Bellomi | Center for Astrophysics | Harvard & Smithsonian
14:50 – 15:15
Turbulence in the ICM: Enhanced Collisionality, Magneto-immutability, and the Extended Cascade
Matthew Kunz | Princeton University
15:15 – 16:00
Coffee Break
16:00 – 16:25
Probing intracluster medium turbulence from deep imaging of Sunyaev-Zel’dovich fluctuations
Adam Remi | Laboratoire Lagrange (OCA)
16:25 – 16:50
Constraining Models of AGN Feedback with Synthetic X-Ray and SZ Observations
Evan Scannapieco | Arizona State University
16:50 – 17:15
Probing ICM turbulence with MHD exascale simulations
Martin Fournier | Hamburg Universitat
17:15 – 18:00
Discussion
Tuesday – 21 July
9:00 – 9:25
XRISM observations of the splash beneath the radio bubble in Ophiuchus
Helen Russell | University of Nottingham
9:25 – 9:50
Insights from simulations -- cool-core destruction and roles of turbulence
Hsiang-Yi Karen Yang | National Tsing Hua University
9:50 – 10:15
Lessons from TNG-Cluster: from cool cores, cavities and shocks to the interpretation of XRISM observations
Annalisa Pillepich | Max Planck Institute for Astronomy, Heidelberg
10:15 – 11:10
Coffee Break
11:10 – 11:35
Multiphase AGN Feedback in Clusters of Galaxies as seen by JWST
Julie Hlavacek-Larrondo | Université de Montréal
11:35 – 12:00
Magnetohydrodynamic Precipitation
Mark Voit | Michigan State University
12:00 – 12:25
Journey to the Black Hole: Multiphase Accretion Flows From Galaxy Scales to Accretion Disk Scales
Yuan Li | UMass Amherst
12:25 – 12:40
Posters
12:40 – 14:00
Lunch
14:00 – 14:25
Thermodynamic Imprints of AGN Feedback and the Baryon Cycle in eROSITA Galaxy Groups and Clusters
Esra Bulbul | Max Planck Institute for Extraterrestrial Physics
14:25 – 14:50
Cool cores and multi-phase gas in TNG-Cluster
Dylan Nelson | Heidelberg University
14:50 – 15:15
Heating from jets in cool-core galaxy clusters
Meenakshi M | Leibniz Institute for Astrophysics, Potsdam
15:15 – 16:00
Coffee Break
16:00 – 16:25
Warm dusty molecular gas: disks, flows, filaments
Megan Donahue | Michigan State University
16:25 – 16:50
Can Mixing Layer simulations explain the remarkably constant Hα–X-ray flux ratios in Galaxy Clusters?
Rajsekhar Mohapatra | Princeton University
16:50 – 17:15
Cosmic Rays and Thermal Instability in Cool Core Clusters
Mateusz Ruszkowski | University of Michigan in Ann Arbor
17:15 – 18:00
Discussion
Wednesday – 22 July
9:00 – 9:25
The connection between the X-ray and radio properties of the cluster cores
Maxim Markevitch | NASA GSFC
9:25 – 9:50
Cluster Merger Shocks in Cosmological and Idealized Box Simulations
Dongsu Ryu | UNIST (Ulsan National Institute of Science and Technology)
9:50 – 10:15
Turbulence excitation in cosmological simulations of massive galaxy cluster mergers
Lorenzo Maria Perrone | Leibniz-Institute for Astrophysics Potsdam (AIP)
10:15 – 11:10
Coffee Break
11:10 – 11:35
Unexpected radio halos
Reinout van Weeren | Leiden University
11:35 – 12:00
Lighting up the past: Odd Radio Circles as Tracers of Past Jet activity
Sebastian Heinz | University of Wisconsin-Madison
12:00 – 12:25
Zooming in on radio relics: How relic morphology probes density fluctuations at the edge of galaxy clusters
Joseph Whittingham | Leibniz Institute for Astrophysics Potsdam (AIP)
12:25 – 12:40
Posters
12:40 – 14:00
Lunch
14:00 – 14:25
Discovery of radio emission upstream of giant shock waves in merging galaxy clusters
Kamlesh Rajpurohit | Center for Astrophysics | Harvard & Smithsonian
14:25 – 14:50
Synthetic Radio and X-ray Observations of Shocks in Simulated Binary Mergers
Hyesung Kang | Pusan National University
14:50 – 15:15
Particle acceleration in intracluster shocks
Damiano Caprioli | University of Chicago
15:15 – 16:00
Coffee Break
16:00 – 22:00
Social Program and Dinner
Thursday – 23 July
9:00 – 9:25
Wanted: Simulations of Radio Galaxies and Filaments in the ICM
Lawrence Rudnick | Univ. of Minnesota
9:25 – 9:50
Cosmic-ray transport and energisation in intermittent ICM environments
Robert Ewart | Princeton University
9:50 – 10:15
Cosmic rays in cosmological simulations - bridging scales
Ludwig Böss | The University of Chicago
10:15 – 11:10
Coffee Break
11:10 – 11:35
Mostly thermal and mostly non-thermal ICM
Eugene Churazov | Max Planck Institute for Astrophysics
11:35 – 12:00
Particle acceleration in astrophysical shocks: from electrons to cosmic rays
Anatoly Spitkovsky | Princeton University
12:00 – 12:25
Particle acceleration and transport in galaxy clusters and large scale structures
Gianfranco Brunetti | INAF- Istituto di Radioastronomia
12:25 – 12:40
Posters
12:40 – 14:00
Lunch
14:00 – 14:25
The interaction of M86 with the Virgo cluster
Jeremy Sanders | Max Planck Institute for Extraterrestrial Physics (MPE)
14:25 – 14:50
Transport in the intracluster medium
Prakriti Palchoudhury | University of Oxford
14:50 – 15:15
The PICO-Cluster Project: cluster sample, magnetic field growth, and weakly collisional effects
Christoph Pfrommer | Leibniz Institute for Astrophysik Potsdam
15:15 – 16:00
Coffee Break
16:00 – 16:25
Ram pressure stripped tails in galaxy clusters
Ming Sun | University of Alabama in Huntsville
16:25 – 16:50
A multi-phase paradigm for turbulent heating and CR transport: CGL simulations and next steps
Stephen Majeski | JILA, University of Colorado and NIST
16:50 – 17:15
Lower Decks: Galaxy Cluster Physics in the Local Universe
Klaus Dolag | USM/LMU
17:15 – 18:00
Discussion
Friday – 24 July
9:00 – 9:25
Bound or blown: the fate of hot gas in galaxy groups
Dominique Eckert | University of Geneva
9:25 – 9:50
Old AGN plasma in galaxy groups
Marisa Brienza | IRA-INAF
9:50 – 10:15
Scale dependent dynamics in multiphase and magnetized turbulence
Philipp Grete | University of Hamburg
10:15 – 11:10
Coffee Break
11:10 – 11:35
A XRISM view of chemical enrichment in galaxy clusters
Francois Mernier | IRAP
11:35 – 12:00
Bridging Scales: Coupling the galactic nucleus to the larger cosmic environment
Kung-Yi Su | CIERA, Northwestern University
12:00 – 12:25
The topology of the magnetic field in Abell 2255 out its virial radius
Andrea Botteon | INAF-IRA
12:25 – 12:40
Posters
12:40 – 14:00
Lunch
14:00 – 14:25
Effects of ICM Turbulence on Magnetic Flux and Polarization Properties
Hui Li | Los Alamos National Laboratory
14:25 – 14:50
TBA
14:50 – 15:15
TBA
15:15 – 16:00
Coffee Break
16:00
End
Posters
Anomalous resistivity in weakly collisional plasma
Aikya Banerjee | University of Oxford
SBI inference of ICM thermodynamics
Joey Braspenning | Max Planck Institute for Astronomy
Turbulence in the ICM: what is XRISM really measuring?
Dimitris Chatzigiannakis | MPIA
Radio emission in MACSJ0018
Paola Dominguez Fernandez | Harvard University
Gas Uplift by AGN Bubbles with Magnetic Fields and Anisotropic Transport
Matthew Goodbred | Princeton University
The evolving ICM: XRISM insights into kinematic and non-equilibrium physics in merging clusters
Annie Heinrich | University of Chicago
Beyond the Spherical Cow: Multiphase Gas Survival in Realistic Cluster Environments
Fernando Hidalgo Pineda | Max Planck Institute for Astrophysics
Simulating realistic morphologies of FRI jets with self-regulated AGN feedback
Léna Jlassi | Leibniz Institute for Astrophysics (AIP)
Automated Search for X-ray Cavities using Deep Learning
Martin Kolář | Masaryk University
“Brick” or “Mist”? Investigating Multiphase Gas Dynamics in Cool-core Galaxy Clusters
Yi-Yang Li | National Tsing Hua University
Viscous or Turbulent? The XRISM Puzzle of Coma
Tirso Marin-Gilabert | Center for Astrophysics | Harvard & Smithsonian
Resolving AGN Feedback in Cluster Cores with XRISM and Chandra
Hannah McCall | University of Chicago
Exploring shock structures in Cosmic Web
Barbora Miklošová | Masaryk University
Magnetic Fields in Proto-clusters
Annalisa Pagliotta | University of Bologna, INAF - IRA
Missing metals in the core of the Centaurus cluster
Tomas Plsek | Masaryk University
Direct observations of AGN-driven feedback: dynamics and ionization of the filaments in M87
Camille Poitras | Université Laval
Role of magnetic Fields in AGN-CGM interactions in massive galaxies at halo masses ∼10^13.5 M⊙
Deovrat Prasad | Cardiff University, UK
AGN feedback as a driver of spiral-like gas structures and cold fronts in cool-core clusters
Majidul Rahaman | National Tsing Hua University, Taiwan
Turbulent Drivers of Multiphase Structure in the ICM: Insights from TNG Cluster simulations
Bipradeep Saha | Max Planck Institute for Astronomy
Exploring a cosmic ray inverse-Compton origin to the SZ-to-X-ray pressure deficit in the cool core cluster ZwCl 3146
Emily Silich | Caltech
Magnetization of Galaxy Protoclusters at High Redshift
Larissa Tevlin | Leibniz Institute for Astrophysics Potsdam
Two-Phase Structure of Synchrotron-Cooling-Unstable Relativistic Plasma
Agnieszka Wierzchucka | University of Oxford
Simulating jets in a turbulent ICM: toward reproducing synchrotron-emitting filaments
Francesca Zanetti | INAF-IRA and University of Bologna