CMB Anisotropy Measurements with the Degree Angular Scale Interferometer (DASI)

Details CMB Anisotropy Measurements with the Degree Angular Scale Interferometer (DASI) CMB Anisotropy Measurements with the Degree Angular Scale Interferometer (DASI)

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.5501c&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #55.01; Bulletin of the American Astronomical Society, Vol. 32, p.1496

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Degree Angular Scale Interferometer (DASI) is a 13-element array of horns operating at 26 - 36 GHz designed explicitly to image anisotropy in the Cosmic Microwave Background radiation and to determine its angular power spectrum over the range 140 < l < 920. DASI was deployed sucessfully at the Amudsen-Scott South Pole station last Austral Summer (December 1999 - January 2000) and has collected high quality data throughout the Austral Winter. After a brief overview of the instrument and its capabilities, the talk will focus on the observations and on the results of the data analysis. DASI is funded by NSF-OPP via the Center for Astrophysical Research in Antarctica, a NSF STC.

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