Measurements of anisotropies in the Cosmic Microwave Background Radiation on scales of half a degree

Details Measurements of anisotropies in the Cosmic Microwave Background Radiation on scales of half a degree Measurements of anisotropies in the Cosmic Microwave Background Radiation on scales of half a degree

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995yera.conf...23o&link_type=abstract

The XXVIIth Young European Radio Astronomers Conference, ed. D.A. Green and W. Steffen, in association with Cambridge University

Astronomy and Astrophysics

Astronomy

Scientific paper

Deep observations of a field have been carried out at 13.5 GHz with the Cosmic Anisotropy Telescope at Cambridge. After removal of foreground radio sources brighter than 10 mJy, using the Ryle Telescope, the resulting map shows evidence for residual structure on a scale of approximately half a degree with rms variation of 18 mJy. Multi-frequency measurements will be used in the future to discriminate between Galactic and cosmic microwave background radiation (CMBR) components of this anisotropy.

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