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Preliminary separation of galactic and cosmic microwave emission for the COBE Differential Microwave Radiometer
The Astrophysical Journal1992Vol. 396, pp. L7–L7
Citations Over TimeTop 1% of 1992 papers
C. L. Bennett, G. F. Smoot, G. Hinshaw, E. L. Wright, A. Kogut, Giovanni De Amici, S. S. Meyer, R. Weiß, D. T. Wilkinson, S. Gulkis, M. Janssen, N. W. Boggess, E. S. Cheng, M. G. Hauser, T. Kelsall, John C. Mather, Jr. Moseley S. H., T. L. Murdock, R. F. Silverberg
Abstract
Preliminary models of microwave emission from the Milky Way Galaxy based on COBE and other data are constructed for the purpose of distinguishing cosmic and Galactic signals. Differential Microwave Radiometer (DMR) maps, with the modeled Galactic emission removed, are fitted for a quadrupole distribution. Autocorrelation functions for individual Galactic components are presented. When Galactic emission is removed from the DMR data, the residual fluctuations are virtually unaffected, and therefore they are not dominated by any known Galactic emission component.
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