Observations of the anisotropy in the cosmic microwave background by the FIRS, SK93, and MSAM-I experiments

Details Observations of the anisotropy in the cosmic microwave background by the FIRS, SK93, and MSAM-I experiments Observations of the anisotropy in the cosmic microwave background by the FIRS, SK93, and MSAM-I experiments

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cwru.rept.....k&link_type=abstract

Technical Report, Case Western Reserve Univ. Cleveland,OH United States

Astronomy and Astrophysics

Astronomy

Anisotropy, Background Radiation, Sky Surveys (Astronomy), Polarization (Waves), Radiometric Resolution, Frequency Ranges, Infrared Astronomy, Cosmic Rays, Autocorrelation, Infrared Radiometers, Microwave Radiometers, Radiometric Correction

Scientific paper

The observations and results from the FIRS, SK93, and MSAM-1, experiments are discussed. These experiments search for anisotropy in the cosmic microwave background over a range in angular scale from 180 deg to 0.5 deg and a range in frequency from 26 to 680 GHz. Emphasis is placed on the observing strategy and potential systematic errors. Contamination of the data by galactic sources is addressed. Future directions are indicated. The results for all three experiments, as found by us and others, are given in the context of the standard CDM model, QCDM, and the model-independent band-power estimates.

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