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Sensitivity of a bolometric interferometer to the cosmic microwave backgroud power spectrum

2008/07/31 by J. -Ch. Hamilton, J.-Ch. Hamilton, R. Charlassier +4 · 1 citation
Physics and Astronomy · #Electrical and Electromagnetic Research #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810504

published as A&A 491, 923-927 (2008) · 5 pages, 3 figures. This last version matches the published version (Astronomy and Astrophysics 491 3 (2008) 923-927). Sensitivity of Heterodyne Interferometers modified by a factor of two

openalex publication_date 2008/10/07 · arxiv created 2008/11/28 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Context. The search for B-mode polarization fluctuations in the Cosmic Microwave Background is one of the main challenges of modern cosmology. The expected level of the B-mode signal is very low and therefore requires the development of highly sensitive instruments with low systematic errors. An appealing possibility is bolometric interferometry.

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