A Search for Small-Scale Anisotropy in the Cosmic Microwave Background

Details A Search for Small-Scale Anisotropy in the Cosmic Microwave Background A Search for Small-Scale Anisotropy in the Cosmic Microwave Background

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...186.5605d&link_type=abstract

American Astronomical Society, 186th AAS Meeting, #56.05; Bulletin of the American Astronomical Society, Vol. 27, p.889

Astronomy and Astrophysics

Astronomy

Scientific paper

Five overlapping regions are observations at 90 GHz with the White Dish telescope operating at the South Pole. Harmonic analysis of the temperature fluctuations reveals a 204 mu K peak-to-peak difference in one of the five regions. Assuming the signal is due to cosmic background anisotropy, the 90-percent confidence limit on gaussian-correlated anisotropy is Delta T = 3.7(+4.6}_{-1.4) TCMB. We review efforts underway to identify the origin of the source.

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