Planck-HFI focal plane concept

Bruno Maffei; Peter A.R. Ade; James J. Bock; J. Brossard; Emily M. Gleeson; Jean-Michel Lamarre; Andrew E. Lange; Yu-Ying Longval; John Anthony Murphy; Giampaolo Pisano; Jean-Loup Puget; I. Ristorcelli; Rashmi V. Sudiwala; Vladimir B. Yurchenko

doi:10.1117/12.552577

12 October 2004 Planck-HFI focal plane concept

Bruno Maffei, Peter A.R. Ade, James J. Bock, J. Brossard, Emily M. Gleeson, Jean-Michel Lamarre, Andrew E. Lange, Yu-Ying Longval, John Anthony Murphy, Giampaolo Pisano, Jean-Loup Puget, I. Ristorcelli, Rashmi V. Sudiwala, Vladimir B. Yurchenko

Author Affiliations +

Proceedings Volume 5487, Optical, Infrared, and Millimeter Space Telescopes; (2004) https://doi.org/10.1117/12.552577
Event: SPIE Astronomical Telescopes + Instrumentation, 2004, Glasgow, United Kingdom

Abstract

The future ESA space mission Planck Surveyor mission will measure the Cosmic Microwave Background temperature and polarisation anisotropies in a frequency domain comprised between 30GHz and 1THz. On board two instruments, LFI based on HEMT technology and HFI using bolometric detectors. We present the optical solutions adopted for this mission, in particular the focal plane design of HFI, concept which has been applied already to other instruments such as the balloon borne experiment Archeops.

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Bruno Maffei, Peter A.R. Ade, James J. Bock, J. Brossard, Emily M. Gleeson, Jean-Michel Lamarre, Andrew E. Lange, Yu-Ying Longval, John Anthony Murphy, Giampaolo Pisano, Jean-Loup Puget, I. Ristorcelli, Rashmi V. Sudiwala, and Vladimir B. Yurchenko "Planck-HFI focal plane concept", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.552577

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