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ARCADE: Absolute radiometer for cosmology, astrophysics, and diffuse emission

2006/09/13 by A. Kogut, D. J. Fixsen, D. Fixsen +13 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Black-body radiation #Cosmic background radiation #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Optics #Physics #Radiation #Radio Astronomy Observations and Technology #Radiometer #Universe #Wavelength #astro-ph

paper · pdf · doi:10.1016/j.newar.2006.09.023

published as New Astron.Rev. 50 (2006) 925-931 · 12 pages, 6 figures. Proceedings of the Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006, to be published in New Astronomy Reviews

arxiv created 2006/09/13 · openalex publication_date 2006/11/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE) is a balloon-borne instrument designed to measure the temperature of the cosmic microwave background at centimeter wavelengths. ARCADE searches for deviations from a blackbody spectrum resulting from energy releases in the early universe. Long-wavelength distortions in the CMB spectrum are expected in all viable cosmological models. Detecting these distortions or showing that they do not exist is an important step for understanding the early universe. We describe the ARCADE instrument design, current status, and future plans.

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