Kavli Affiliate: Luis Ho | Summary:A significant puzzle in extragalactic astronomy is the scarcity of Little Red Dots (LRDs) at $z < 3$, compared to their higher abundance at earlier epochs. To understand this transition, we investigate the cosmic evolution of LRD environments. We measure the overdensity for LRDs and the general galaxy population at […]
Continue.. Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass