Dark Energy Survey Cluster Cosmology Constraints with Simulation-based Forward Modeling

Explore advanced cosmological constraints derived from galaxy cluster observations in this 13-minute conference talk by Andres Salcedo from the University of Arizona's Steward Observatory. Learn about simulation-based forward modeling techniques applied to Dark Energy Survey data to extract cosmological parameters from galaxy cluster populations. Discover how researchers combine observational data with sophisticated computational models to better understand dark energy and the large-scale structure of the universe. Examine the methodological approaches used to analyze cluster mass distributions and their implications for cosmological models. Gain insights into cutting-edge techniques that bridge observational astronomy with theoretical cosmology, presented as part of the New Synergies in Multi-Probe Cosmology conference at the Kavli Institute for Theoretical Physics.