QUIJOTE Experiment: status of telescopes and instrumentation
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Identificadores
URI: http://hdl.handle.net/10902/11122DOI: 10.1117/12.2233225
ISSN: 0277-786X
ISSN: 1996-756X
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Pérez de Taoro, María del Rosario Ángeles; Aguiar González, Marta; Cózar Castellano, Juan; Génova Santos, Ricardo Tanausú; Gómez Reñasco, María Francisca; Hoyland, Roger J.; Peláez Santos, Alba Eva; Poidevin, Frédérick; Tramonte, Denis; Rebolo López, Rafael; Casas Reinares, Francisco Javier






Fecha
2016Derechos
Copyright 2016 Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Publicado en
Proceedings of SPIE, 2016, 9906, 99061K
Ground-based and Airborne Telescopes VI, Edinburgh, United Kingdom, 2016
Editorial
SPIE Society of Photo-Optical Instrumentation Engineers
Enlace a la publicación
Palabras clave
Microwaves
Polarization
CMB
B-modes
Telescopes
Instrumentation
Cryogenics
Temperature control
Resumen/Abstract
The QUIJOTE Experiment (Q-U-I JOint TEnerife) is a combined operation of two telescopes and three instruments working in the microwave band to measure the polarization of the Cosmic Microwave Background (CMB) from the northern hemisphere, at medium and large angular scales. The experiment is located at the Teide Observatory in Tenerife, one of the seven Canary Islands (Spain). The project is a consortium maintained by several institutions: the Instituto de Astrofísica de Canarias (IAC), the Instituto de Física de Cantabria (IFCA), the Communications Engineering Department (DICOM) at Universidad de Cantabria, and the Universities of Manchester and Cambridge. The consortium is led by the IAC.
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