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Título: | The QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions |
Autor: | Rubiño-Martín, J. A.; Rebolo López, Rafael CSIC ORCID; Aguiar-González, Marta; Martínez-González, Enrique CSIC ORCID ; Barreiro, R. Belén CSIC ORCID ; Casas-Reinares, F. J. CSIC ORCID ; Diego, José María CSIC ORCID ; Fernández-Cobos, R. CSIC ORCID ; Herranz, D. CSIC ORCID ; López-Caniego, M. CSIC ORCID; Ortiz, David CSIC ORCID; Vielva, Patricio CSIC ORCID ; Artal, Eduardo; Villa, Enrique | Palabras clave: | Polarisation Cosmological parameters Early Universe Telescopes Cosmic microwave background |
Fecha de publicación: | 2012 | Editor: | The International Society for Optics and Photonics | Citación: | Proceedings of SPIE 8444: 84442Y (2012) | Resumen: | The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment will operate at the Teide Observatory with the aim of characterizing the polarisation of the CMB and other processes of Galactic and extragalactic emission in the frequency range of 10–40 GHz and at large and medium angular scales. The first of the two QUIJOTE telescopes and the first multi-frequency (10–30 GHz) instrument are already built and have been tested in the laboratory. QUIJOTE-CMB will be a valuable complement at low frequencies for the Planck mission, and will have the required sensitivity to detect a primordial gravitational-wave component if the tensor-to-scalar ratio is larger than r = 0.05. | Descripción: | Trabajo presentado a la conferencia: "Ground-based and Airborne Telescopes IV" (Poster session: Concepts for future telescopes) celebrada en Amsterdam (Holanda) el 1 de julio de 2012.-- et al. | Versión del editor: | http://dx.doi.org/10.1117/12.926581 | URI: | http://hdl.handle.net/10261/109135 | DOI: | 10.1117/12.926581 | Identificadores: | doi: 10.1117/12.926581 issn: 0277-786X e-issn: 1996-756X |
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QUIJOTE-CMB.pdf | 7,65 MB | Unknown | Visualizar/Abrir |
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