In-Person
Ivana Barisic (UC Davis)
Lunch talk: MSA-3D: Radial Dust Attenuation Diversity and Star Formation Activity at the Epoch of Thin Disk Emergence (z∼1)
Overview
Spatially resolved profiles of star formation offer valuable insight into galaxy growth and structural evolution. Integral field spectroscopy (IFS) at high angular resolution is essential for resolving the underlying structure, and identifying mechanisms regulating structural evolution.