Main Page | Science Goals | Group Members | Publications | Caltech Home
Project Overview | Instrument Description | Project Team | Publications | Links



BICEP Instruments

click on thumbnail for full image
Figure 6: BICEP mount and environmental enclosure. The mount allows the receiver to continuously rotate about the optical axis and periodically toggle by 180 degrees in azimuth.
BICEP will combine a 20 cm primary aperture, refractive optics, and a polarization-sensitive detector array cooled to 250 mK to achieve 1 deg and 0.7 deg beams at 100 GHz and 150 GHz, respectively, over a 20-degree diameter field-of-view.

More information on the instruments is available in this paper.  
 

Copyright © Caltech Observational Cosmology, 2002   -   Last updated June 2002