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Registration has been CLOSED for in-person attendees!
To attend virtually, please reach out to ccaadmin@flatironinstitute.org. A Zoom link will be sent upon approval from event organizers.
A recording of this event will be posted to our website for later viewing.
Event Overview
The goal of this meeting is to bring together theoreticians, modelers, and observers to discuss the challenges and identify promising paths forward for the next generation of observatories, focusing on the next generation Very Large Array (ngVLA). The formation of planetary systems, the evolution of galaxies, and the observation of electromagnetic counterparts of gravitational wave events will be fertile grounds for discovery in the next decades and are core science goals for the ngVLA. The challenge to simulators is to develop predictive models that can be accurately compared against observations, while observers need to generate measurements that can effectively constrain the models. What are the key observables that will allow us to disentangle evolutionary processes and formation and generation mechanisms? What is needed to improve the current generation of theories and models, in order to produce accurate predictions of observable parameters? What types of observational capabilities and programs will be needed to constrain the theories? What are the computational and data challenges, and how can they be overcome?
This meeting will take place for three days at the Simons Foundation's Flatiron Institute in Manhattan, New York. We particularly encourage the participation of early career scientists. The meeting will be in person, but talks will be recorded and made widely available. It will be structured to stimulate dynamic, real-time interactions concerning model development and identification of future observations.
Zachary Davis: Modeling Turbulent Heating Inside of Blazars
Antonio Hales: Millimeter Studies of Eruptive Stars
Kevin Flaherty: Evidence for Turbulence Around IM Lup as Revealed by ALMA
Eva Duran Camacho: Constraining the Milky Way structure through numerical models
Nathan Roth: The Next Generation of the Protoplanetary Disk-Comet Connection: Synergistic Studies of Disk Midplane Chemistry and Cometary Atmospheres with ngVLA
Guochao Sun: Simulating Multi-Tracer Intensity Mapping of Cosmic Dawn and Reionization Eras with LIMFAST
Wenrui Xu: How Massive Are Typicall Protostellar Disks? Insights From a Synergy Between Theory and Observation
Valentina La Torre: Parameter Estimation with SOM for Large Survey Datasets
Duncan Brown & Alessandra Corsi: Observing Black Holes and Neutron Stars Throughout Time with Cosmic Explorer
Cristiano Longarini: Kinematical Imprints of Self Gravity and Gravitational Instability
Tirso Marin Gilabert: The Effect of Braginskii Viscosity in the Intracluster Medium
Jan-Willem Steeb: SiRIUS: Simulation of Radio Interferometry from Unique Sources
Allison Towner: Identifying Previous Generations of Shocks in MYSOs
Ashkbiz Danehkar: Hydrodynamic Simulations of Starburst-driven Superwinds and Superbubbles
Massimo Ricotti: Multiscale Radiation Hydrodynamic Simulation of Star Clusters Formation Across Cosmic Time
Yuong-Dae Jung: Atomic Data for Shannon Entropy in Astrophysical Compact Objects
Jeff Jennings: Super-resolution Imaging with Frankenstein
Sumit Sarbadhicary: Supernova Progenitors and Feedback From the Most Detailed Radio Images of Local Group Galaxies
Frederick Groth: Impact of the Hydrodynamical Scheme on High Resolution Simulations of Structure Formation
Elie Pattie: A Radio Survey in the Galactic Bulge