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The cosmic microwave background spectrum measured by the FIRAS instrument on the COBE satellite is the most precisely measured black body spectrum in nature. The data points and error bars on this graph are obscured by the theoretical curve.
 

There are 5 summaries on Cosmic microwave background radiation.

Encyclopedia and Summary Information
summary from source:
Cosmic Microwave Background Radiation Summary
837 words, approx. 3 pages
In 1965, American physicists Arno Penzias (1933–) and Robert Wilson (1936–) announced the discovery of microwave radiation, which uniformly filled the sky and had a blackbody temperature of about 3.5K. The pair had been testing a new...
summary from source:
Microwave Background Radiation Summary
639 words, approx. 2 pages
In 1964, a pair of radio astronomers, American physicist Robert Wilson (1936-) and German-born physicist Arno Penzias, working for the Bell Telephone Laboratories in Holmdel, New Jersey, stumbled upon the best evidence in existence to support the big...
summary from source:
Cosmic Background Radiation Summary
495 words, approx. 2 pages
The 1965 discovery of cosmic background radiation by Arno A. Penzias and Robert W. Wilson provided important evidence in support of big bang based cosmological models first proposed after American astronomer Edwin Hubble's (1889-1953) discovery that...
summary from source:
Cosmic Background Radiation Summary
57 words, approx. 0 pages
Electromagnetic radiation, mostly in the microwave range, believed to be the highly redshifted residual effect (&see; redshift) of the explosion billions of years ago from which, according to the big-bang model, the universe was created. It was...
summary from source:
Cosmic microwave background radiation Summary
5,386 words, approx. 18 pages
In cosmology, the cosmic microwave background radiation (most often abbreviated CMB but occasionally CMBR, CBR or MBR, also referred to as relic radiation) is a form of electromagnetic radiation discovered in 1965 that fills the entire universe.[1] It...


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