I'm a passionate researcher interested in the study of galaxy formation and evolution. My current research involves the search for dust emission from SC4K LAEs at redshift 2 to 6 in the COSMOS field. Using a sample of ~4000 SC4K LAEs and SCUBA-2 850 micron data from the JCMT telescope, I'm working to deepen our understanding of the mechanisms of star formation and the evolution of galaxies.
Dust emission from Lyman alpha emitter (LAE) galaxies is an exciting area of research in observational Astrophysics. LAEs are a special class of galaxies that are characterized by their strong emission lines in the Lyman alpha wavelength. These galaxies are thought to be actively forming stars and represent an important population for studying the early Universe. The dust emission from LAEs is of particular interest as it provides insights into the distribution of dust within these galaxies. By studying the dust content of LAEs, we can gain a better understanding of the mechanisms of star formation and the evolution of galaxies. The submillimeter data obtained from telescopes such as the JCMT are particularly useful for studying dust emission from LAEs, as they allow for a detailed analysis of the dust properties and distribution within these galaxies. Ultimately, research into dust emission from LAEs has the potential to deepen our understanding of the Universe and the processes that shape it.