Bibcode
Sánchez-de-la-Rosa, V.; Vega-Moreno, A.; Cózar-Castellano, J.; Aguiar-González, M.; Galtress, A.; Génova-Santos, R.; Gómez-Reñasco, F.; Hoyland, R.; Martinis, L.; Melhuish, S. J.; Pérez-de Taoro, M. R.; Piccirillo, L.; Rebolo-López, R.; Rubiño-Martín, J. A.; Viera-Curbelo, T. A.
Referencia bibliográfica
Proceedings of the SPIE, Volume 9914, id. 99142N 15 pp. (2016).
Fecha de publicación:
7
2016
Número de citas
0
Número de citas referidas
0
Descripción
The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment is operating at the
Teide Observatory with the aim of characterizing the polarization of the
CMB and other processes of Galactic and extragalactic emission in the
frequency range of 10-40GHz and at large and medium angular scales. The
QUIJOTE CMB experiment consists of two telescopes installed inside a
single enclosure, and three instruments, the MFI (multi-frequency
10-30GHz), the TGI (26-36 GHz) and the FGI (37-47 GHz). The first
QUIJOTE telescope and the MFI instrument have been in operation at the
Observatory since November 2012. In this poster we present the TGI
cryostat and optomechanics status, including their design, MAIT, and
thermal clamp developments.