2001/12/07 by F. Villa, M. Bersanelli, C. Burigana +7 · 3 citations
Physics and Astronomy · #Cosmology and Gravitation Theories #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph
paper · pdf · doi:10.1063/1.1475633
On behalf of the Planck collaboration. 5 pages, 4 figures. The following article has been submitted for publication in the AIP Proceedings of the Workshop on "Experimental Cosmology at millimeter wavelengths", Cervinia, Italy, 9-13 July 2001
arxiv created 2001/12/07 · openalex publication_date 2002/01/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/29
In this paper we present an overview of the Telescope designed for ESA’s mission dedicated to map the Cosmic Microwave Background Anisotropies and Polarization. Two instrument, LFI and HFI, operate in an overall frequency range between 25 and 900 GHz and share the focal region of the 1.5 meter optimized aplanatic telescope. The optimization techniques adopted for the optical design and the telescope characteristic are reported and discussed.