Research
Main content start
What are we interested in?
Introduction to Cosmology
As cosmologists we are interested in the origin and evolution of the Universe. For the first 360,000 years the Universe was in a very hot and dense state. Today we can measure the afterglow from the hot plasma in the early Universe, called the Cosmic Microwave Background (CMB).
What do we work on?
CMB experiments
How to make the most precise cosmological measurements?
Instrumentation for Radio Astronomy
How to learn about our Universe from the data?