Abstract
Astrophysical experiments dedicated to the study of the Cosmic Microwave Background are in needs of very well defined beam shape in order to get ail accurate re-construction of the anisotropies power spectrum. These beams have to be carefully designed, but also properly characterised. Some of these instruments will be located in a cryostat for which filters and windows are necessary, and the effects of these additional optical components oil the beam shape need to be taken into account. We present here, measurements of such effects on the co- and cross-polarisation radiation patterns of corrugated horns using a Vector Network Analyser.
Original language | English |
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Title of host publication | Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV |
Editors | W D Duncan, W S Holland, S Withington, J Zmuidzinas |
Publisher | SPIE |
Pages | H202-H202 |
Volume | 7020 |
ISBN (Print) | 0277-786X 978-0-8194-7230-4 |
Publication status | Published - 2008 |
Event | Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV - Marseille, FRANCE Duration: 26 Jun 2008 → 28 Jun 2008 |
Conference
Conference | Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV |
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City | Marseille, FRANCE |
Period | 26/06/08 → 28/06/08 |
Keywords
- CMB experiments
- corrugated feedhorns
- systematic effects
- co and
- cross-polarisation beams
- Astronomy & Astrophysics
- Instruments & Instrumentation
- Optics