N. Goeckner-Wald

Researchers analyze the kSZ effect to learn about cosmic reionization.

Upcoming studies aim to refine our view of the universe using SPT-3G data.

The 220/270 GHz receiver aids in studying the Cosmic Microwave Background.

Astronomers monitor satellite emissions to understand their impact on cosmic observations.

ML enhances pointing precision at the South Pole Telescope for better cosmic observations.