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Preliminary separation of galactic and cosmic microwave emission for the COBE Differential Microwave Radiometer

Journal Article · · Astrophysical Journal; (United States)
DOI:https://doi.org/10.1086/186505· OSTI ID:6893132
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  1. NASA, Goddard Space Flight Center, Greenbelt, MD (United States) Lawrence Berkeley Laboratory, CA (United States) California, University, Berkeley (United States) Universities Space Research Association, Boulder, CO (United States) California, University, Los Angeles (United States) MIT, Cambridge, MA (United States) Princeton University, NJ (United States) JPL, Pasadena, Ca (United States)
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. 42 refs.
OSTI ID:
6893132
Journal Information:
Astrophysical Journal; (United States), Journal Name: Astrophysical Journal; (United States) Vol. 396:1; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English