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Spectrum of the cosmic background radiation at millimeter wavelengths
The spectrum of the cosmic background radiation in five frequency bands extending from 2.3 to 11.0 cm with a balloon-borne liquid-helium-cooled photometer. The photometer compares the flux from the sky to the flux from an internal blackbody at 3.2 K. All five measurements are consistent with tempera...
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Published in: | Physical review letters 1985-07, Vol.55 (3), p.332-335 |
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container_title | Physical review letters |
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creator | Peterson, J. B. Richards, P. L. Timusk, T. |
description | The spectrum of the cosmic background radiation in five frequency bands extending from 2.3 to 11.0 cm with a balloon-borne liquid-helium-cooled photometer. The photometer compares the flux from the sky to the flux from an internal blackbody at 3.2 K. All five measurements are consistent with temperatures in the range 2.78 + or = 0.11 K, which is in good agreement with tempratures measured at lower frequencies. No significant deviation from a thermal spectrum was found. |
doi_str_mv | 10.1103/PhysRevLett.55.332 |
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source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Astronomy Cosmology Earth, ocean, space Exact sciences and technology Observational cosmology (including hubble constant, distance scale, cosmological constant, early universe, etc.) Space Radiation Stellar systems. Galactic and extragalactic objects and systems. The universe |
title | Spectrum of the cosmic background radiation at millimeter wavelengths |
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