Abstract
We describe the design and performance of a microwave polarimeter used to make precision measurements of polarized astrophysical radiation in three microwave frequency bands spanning 26-36 GHz. The instrument uses cooled HEMT amplifiers in a correlation polarimeter configuration to achieve high sensitivity and long-term stability. The instrument demonstrates long-term stability and has produced the most restrictive upper limits to date on the large angular scale polarization of the 2.7 K cosmic microwave background radiation.
Original language | English |
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Pages (from-to) | 1-20 |
Number of pages | 19 |
Journal | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES |
Volume | 144 |
Issue number | 1 |
DOIs | |
Publication status | Published - Jan 2003 |
Keywords
- Cosmic microwave background
- Cosmology: observations
- Instrumentation: polarimeters
- Radio continuum: general