Sensitive measurement of fluctuations in the cosmic microwave background

R. D. Davies, A. N. Lasenby, R. A. Watson, E. J. Daintree, J. Hopkins, J. Beckman, J. Sanchez-Almeida, R. Rebolo

    Research output: Contribution to journalArticlepeer-review

    Abstract

    Extensive high sensitivity observations of the cosmic microwave background have been made on an angular scale of 8° covering a substantial fraction of the northern sky. An observed anisotropy in the sky emission at a level of δT/T = 3.7×l0-5 has been detected (T is temperature). This level should strictly be interpreted as an upper limit to the cosmic microwave background fluctuations. It is possibly the direct imprint of density perturbations in the early Universe. © 1987 Nature Publishing Group.
    Original languageEnglish
    Pages (from-to)462-465
    Number of pages3
    JournalNature
    Volume326
    Issue number6112
    DOIs
    Publication statusPublished - 1987

    Keywords

    • TEMPERATURE DISTRIBUTION

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