The QUIJOTE-CMB experiment: studying the polarisation of the galactic and cosmological microwave emissions
- Stepp, Larry M.
- Rubiño-Martín, J. A.
- Rebolo, R.
- Aguiar, M.
- Génova-Santos, R.
- Gómez-Reñasco, F.
- Herreros, J. M.
- Hoyland, R. J.
- López-Caraballo, C.
- Pelaez Santos, A. E.
- Sanchez de la Rosa, V.
- Vega-Moreno, A.
- Viera-Curbelo, T.
- Martínez-Gonzalez, E.
- Barreiro, R. B.
- Casas, F. J.
- Diego, J. M.
- Fernández-Cobos, R.
- Herranz, D.
- López-Caniego, M.
- Ortiz, D.
- Vielva, P.
- Artal, E.
- Aja, B.
- Cagigas, J.
- Cano, J. L.
- de la Fuente, L.
- Mediavilla, A.
- Terán, J. V.
- Villa, E.
- Piccirillo, L.
- Battye, R.
- Blackhurst, E.
- Brown, M.
- Davies, R. D.
- Davis, R. J.
- Dickinson, C.
- Harper, S.
- Maffei, B.
- McCulloch, M.
- Melhuish, S.
- Pisano, Giampaolo
- Watson, R. A.
- Hobson, M.
- Grainge, K.
- Lasenby, A.
- Saunders, R.
- Scott, P.
- Gilmozzi, Roberto
- Hall, Helen J.
DOIAbstract
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 10-40GHz and at large and medium angular scales. The first of the two QUIJOTE telescopes and the first multi-frequency (10-30GHz) 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. © (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloadin...
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