The Cosmic Microwave Background: State of the Art

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Abstract
We review the current status of the cosmic microwave background (CMB) radiation, including a revision of some basic theoretical aspects, a summary of anisotropy detections and CMB experiments, and a description of some relevant characteristics of the microwave foregrounds. We also discuss the different estimators proposed in the literature to detect non-Gaussianity and outline the basis of some reconstruction methods that have been applied to the CMB.

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