DocumentCode :
531640
Title :
Cosmic microwave background polarization receivers: QUIJOTE experiment
Author :
Artal, Eduardo ; De la Fuente, Luisa ; Aja, Beatriz ; Cano, Juan L. ; Villa, Enrique ; Hoyland, Roger ; Rubiño-Martin, J.A. ; Génova, Ricardo
Author_Institution :
Dept. de Ing. de Comun., Univ. de Cantabria, Santander, Spain
fYear :
2010
fDate :
28-30 Sept. 2010
Firstpage :
497
Lastpage :
500
Abstract :
The QUIJOTE (QUI JOint TEnerife) Experiment will characterize the polarization of Cosmic Microwave Background radiation and other galactic and extragalactic emissions in the frequency range from 10 to 30 GHz, and at large angular scales. The polarimeter receivers at 11,13, 17, 19 and 30 GHz are radiometers based on broadband waveguide rotating polar modulators and broadband orthomode transducers. High sensitivity of polarimeters is achieved with very low noise cryogenic amplifiers (Noise temperature <; 15 K in 11-19 GHz channels and <; 20 K in 30 GHz channel). Subsystems test results and integration measurements of front-end and back-end units show wideband operation in all channels.
Keywords :
astronomical polarimetry; polarimeters; radioastronomical techniques; radioastronomy; radiofrequency cosmic radiation; radiotelescopes; CMB polarization receivers; Q U I Joint Tenerife experiment; QUIJOTE experiment; broadband orthomode transducers; broadband waveguide rotating polar modulators; cosmic microwave background; extragalactic emissions; frequency 10 GHz to 30 GHz; polarimeter receivers; radiometers; very low noise cryogenic amplifiers;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Microwave Conference (EuMC), 2010 European
Conference_Location :
Paris
Print_ISBN :
978-1-4244-7232-1
Type :
conf
Filename :
5616610
Link To Document :
بازگشت