Abstract
The far infrared polarimeter with very low instrumental polarization to be employed at MITO telescope to search for calibration sources was presented. The investigation of polarization near the cosmic microwave background (CMB) anisotropy peaks was done. The analysis of problems connected with spurious polarization removing was done and a method for non-gaussian atmospheric fluctuation was presented.
Original language | English (US) |
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Title of host publication | Proceedings of SPIE - The International Society for Optical Engineering |
Editors | S. Fineschi |
Pages | 241-249 |
Number of pages | 9 |
Volume | 4843 |
DOIs | |
State | Published - 2002 |
Externally published | Yes |
Event | Polarimetry in Astronomy - Waikoloa, HI, United States Duration: Aug 25 2002 → Aug 28 2002 |
Other
Other | Polarimetry in Astronomy |
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Country/Territory | United States |
City | Waikoloa, HI |
Period | 8/25/02 → 8/28/02 |
Keywords
- Cosmology: cosmic microwave background
- Instrumentation: interferometers
- Instrumentation: polarimeters
- Telescopes
ASJC Scopus subject areas
- Electrical and Electronic Engineering
- Condensed Matter Physics