Modelling Emission Lines in Cosmological and Galaxy Simulations

Explore the latest advancements in modelling emission lines for cosmological and galaxy simulations in this 35-minute conference talk by Michaela Hirschmann from EPFL. Recorded as part of the "Cosmic Dawn Revealed by JWST" conference at the Kavli Institute for Theoretical Physics, delve into cutting-edge research on the physics of the first stars, galaxies, and black holes. Gain insights into how JWST observations are challenging and refining theoretical models of galaxy formation. Examine key questions about the nature of early stellar populations, star formation histories, and the physical processes shaping early galaxy and black hole evolution. Connect the findings from near-field and deep field observations to enhance understanding of cosmic dawn. Benefit from the collaborative discussions between theorists and observers as they interpret JWST data and its implications for our comprehension of the universe's earliest structures.

Modelling emission lines in cosmological & galaxy simulations (R) ▸ Michaela Hirschmann (EPFL)