Measurements of cosmic background radiation anisotropy at intermediate angular scale
Results from an Antarctic ground-based experiment devoted to the search for fluctuations in the cosmic background radiation (CBR) are presented. We have developed an off-axis telescope with a Gaussian beam response of 50′ FWHM and with a beam-throw adjustable from 0° to 2°. The detector was a 3He bo...
| Main Authors: | , |
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| Format: | Article in Journal/Newspaper |
| Language: | English |
| Published: |
1993
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| Subjects: | |
| Online Access: | https://research.manchester.ac.uk/en/publications/86f1439f-e3c8-4357-845e-e8efce624e5d http://www.journals.uchicago.edu/ApJ |
| Summary: | Results from an Antarctic ground-based experiment devoted to the search for fluctuations in the cosmic background radiation (CBR) are presented. We have developed an off-axis telescope with a Gaussian beam response of 50′ FWHM and with a beam-throw adjustable from 0° to 2°. The detector was a 3He bolometer working at 0.35 K and operating at 2.2 mm wavelength. The data collected show evidence of fluctuations at a level of ΔTrms/T = 4.5 × 10-5 at an angular scale of 40′. The expected fluctuations obtained by extrapolating the COBE result down to this angular scale, in a cold dark matter scenario, are a factor 2.5 lower (1.8 × 10-5). If residual systematic effects or cold galactic dust emission are responsible for the signal detected, our result should be considered as an upper limit to CBR anisotropy. |
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