The main objectives of our DSFG surveys will be to identify and characterize these galaxies (measuring luminosity functions, redshift distributions, correlation functions, etc), and conduct searches for z>5 sources and IR-bright protocluster systems using current and upcoming (sub)millimeter surveys of the southern sky, from the SPT 3G collaboration, the CCAT observatory surveys and the CMB-S4 project.
Type of project: Research – actively recruiting new young researchers
Status: Ongoing
Researchers: Manuel Aravena
Funding source: Basal CATA2