Galactic synchrotron emission at high frequencies
The search for structure in the cosmic microwave background (CMB) needs to take into account the Galactic background contribution. The potential of using existing maps at 408 and 1420 MHz to determine this correction at high frequencies is examined. It is found that a significant part of the high Galactic latitude structure evident in these maps is
Gutierrez, C. M. et al.
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1996