Abstract
We describe the instrumentation, experiment design, and data reduction for the first season of observations with the Degree Angular Scale Interferometer (DASI), a compact microwave interferometer designed to measure anisotropy of the cosmic microwave background (CMB) on degree and subdegree scales (l ≃ 100-900). The telescope was deployed at the Amundsen-Scott South Pole Research Station during the 1999-2000 austral summer, and we conducted observations of the CMB throughout the following austral winter. In its first season of observations, DASI has mapped CMB fluctuations in 32 fields, each 3°.4 across, with high sensitivity.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 28-37 |
| Number of pages | 10 |
| Journal | Astrophysical Journal |
| Volume | 568 |
| Issue number | 1 I |
| DOIs | |
| State | Published - Mar 20 2002 |
Keywords
- Cosmic microwave background
- Cosmology: observations
- Techniques: interferometric
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