Cosmic noon refers to a period in the history of the universe when galaxies were forming stars at their highest rates. This era, which occurred around 10 billion years ago, is a critical time in the evolution of galaxies and the universe as a whole. During cosmic noon, galaxies were actively forming and evolving, leading to the diverse range of galaxy types we see today. Studying this period can provide valuable insights into the processes that govern galaxy formation and evolution, as well as the growth of supermassive black holes at the centers of galaxies. Researchers studying cosmic noon use a variety of tools and techniques, including observational data from telescopes and simulations based on theoretical models. By studying the properties of galaxies during this crucial period in the universe's history, scientists aim to better understand the mechanisms driving cosmic evolution and the formation of the structures we observe in the universe today.