The 170 GHz Survey Large Scale CMBR Anisotropy Measurement

Details The 170 GHz Survey Large Scale CMBR Anisotropy Measurement The 170 GHz Survey Large Scale CMBR Anisotropy Measurement

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.7704g&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #77.04; Bulletin of the American Astronomical Society, Vol. 25, p.928

Astronomy and Astrophysics

Astronomy

Scientific paper

The results of a cross-correlation between the 170 GHz Survey map and the COBE DMR `Fit Technique' reduced Galaxy all-sky map are presented. Because these two experiments use different observing methods, are sensitive to different Galactic components, and use different data reduction methods, the significant cross-correlation indicates that both instruments have observed anisotropies consistent with variations in a 2.7 K emitter. The 170 GHz auto-correlation function is also presented.

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