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CARA Science: White Dish
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Summary
White Dish is one of the
instruments in CARA that study the cosmic
microwave background radiation (CMBR). It was at the Pole
from 1991-1993.
White Dish was a 1.4-meter telescope which measured anisotropies in the
CMBR.
White Dish used a single-mode waveguide composite bolometer from
75-105 GHz.
Results
White Dish was the first of several telescopes built by the
Peterson group at Carnegie Mellon University.
- Tucker, G. S., Griffin, G. S., Nguyen, H. T., Peterson, J. B., 1993,
"A
Search for Small-Scale Anisotropy in the Cosmic Microwave Background",
ApJ, 419, L45.
- A summary
sheet for this experiment.
Photos
For more information
The group has a website at
http://cmbr.phys.cmu.edu/whitedish.html .
White Dish is based at Carnegie-Mellon University.
For more information, contact Jeff Peterson,
jeff@cmbr.phys.cmu.edu .
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