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Near-millimeter spectrum of the microwave background

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/159126· OSTI ID:5849967
A complete description is given of a measurement of the spectrum of the cosmic microwave background (CMB). A fully calibrated, liquid helium cooled, ballon borne spectrophotometer was used to measure the emission spectrum of the night sky over the frequency range from 1.7 to 40 cm/sup -1/. Great care was taken with the instrumental design to avoid radiation from the Earth or the apparatus. The apparatus was calibrated using a blackbody source with a variety of temperatures before and after the flight. The atmospheric emission was subtracted by fitting the data to the spectrum computed from an atmospheric model. The resulting spectral measurements have a flux accuracy of better than 10% of the peak flux of a 3 K blackbody and extend over the frequency range from 2.5 to 24 cm/sup -1/. They show that the spectrum of the CMB peaks at 6 cm/sup -1/ and is approximately that of a blackbody out to several times that frequency. Some deviations from blackbody shape are observed. The measured flux is equivalent to that from a blackbody in the temperature range from 2.88 to 3.09 K. These measurements are combined with previous observations of the CMB to produce a set of data covering three decades in frequency. This data set is compared with various models of the CMB.
Research Organization:
Department of Physics, University of California; and Materials and Molecular Research Division, Lawrence Berkeley Laboratory
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
5849967
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 248:1; ISSN ASJOA
Country of Publication:
United States
Language:
English