OVRO/BIMA SZE Imaging Experiment

Primary Goal: The OVRO/BIMA SZE Imaging experiment was designed to make detailed images of the Sunyaev-Zel'dovich effect in clusters of galaxies and to use these measurements to learn about cluster physics and cosmology

Receiver: 30 GHz HEMT - based receivers


  • OVRO (Owens Valley Radio Observatory) 
  • BIMA (Berkeley Illinois Maryland Array)

Example HR

The Team
Photo Galleries

BIMA                         OVRO 

Near BIMA                 Near OVRO