Observational bounds on the cosmic microwave background anisotropy at small and intermediate angular scale

Details Observational bounds on the cosmic microwave background anisotropy at small and intermediate angular scale Observational bounds on the cosmic microwave background anisotropy at small and intermediate angular scale

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..141v&link_type=abstract

In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 19

Astronomy and Astrophysics

Astrophysics

5

Anisotropy, Cosmology, Microwaves, Relic Radiation, Astronomical Models, Baryons, Dark Matter, Galactic Evolution, Power Spectra

Scientific paper

A way of analyzing cosmic microwave background (CMB) data is presented in order to extract statistically robust upper limits. The analysis, which is based on a likelihood ratio test, is applied to data from three CMB anisotropy experiments. The statistical significance of the upper limits obtained by the method and the constraints that can be imposed on the density parameter and the baryonic abundance of flat and open CDM models are discussed.

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