We present the current status of the QUIJOTE (Q-U-I JOint TEnerife) CMB Experiment, a new instrument which will start operations early in 2009 at Teide Observatory with the aim of characterizing the polarization of the CMB and other processes of galactic and extragalactic emission in the frequency range 10-30GHz and at large angular scales. QUIJOTE 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 D 0:05. © Springer-Verlag Berlin Heidelberg 2010.

The QUIJOTE CMB experiment / Rubino-Martin, J. A.; Rebolo, R.; Tucci, M.; Genova-Santos, R.; Hildebrandt, S. R.; Hoyland, R.; Herreros, J. M.; Gomez-Renasco, F.; Lopez Caraballo, C.; Martinez-Gonzalez, E.; Vielva, P.; Herranz, D.; Casas, F. J.; Artal, E.; Aja, B.; Dela Fuente, L.; Cano, J. L.; Villa, E.; Mediavilla, A.; Pascual, J. P.; Piccirillo, L.; Maffei, B.; Pisano, G.; Watson, R. A.; Davis, R.; Davies, R.; Battye, R.; Saunders, R.; Grainge, K.; Scott, P.; Hobson, M.; Lasenby, A.; Murga, G.; Gomez, C.; Gomez, A.; Arino, J.; Sanquirce, R.; Pan, J.; Vizcarguenaga, A.; Etxeita, B.. - (2010), pp. 127-135. (Intervento presentato al convegno 8th Scientific Meeting of the Spanish Astronomical Society, SEA 2008 tenutosi a Santander, esp) [10.1007/978-3-642-11250-8_12].

The QUIJOTE CMB experiment

Pisano G.;
2010

Abstract

We present the current status of the QUIJOTE (Q-U-I JOint TEnerife) CMB Experiment, a new instrument which will start operations early in 2009 at Teide Observatory with the aim of characterizing the polarization of the CMB and other processes of galactic and extragalactic emission in the frequency range 10-30GHz and at large angular scales. QUIJOTE 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 D 0:05. © Springer-Verlag Berlin Heidelberg 2010.
2010
8th Scientific Meeting of the Spanish Astronomical Society, SEA 2008
Cosmic Microwave Background radiation, B-Modes, Instrumentation, Polarimetry, Millimetre waves, Microwave receivers, Polarization
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
The QUIJOTE CMB experiment / Rubino-Martin, J. A.; Rebolo, R.; Tucci, M.; Genova-Santos, R.; Hildebrandt, S. R.; Hoyland, R.; Herreros, J. M.; Gomez-Renasco, F.; Lopez Caraballo, C.; Martinez-Gonzalez, E.; Vielva, P.; Herranz, D.; Casas, F. J.; Artal, E.; Aja, B.; Dela Fuente, L.; Cano, J. L.; Villa, E.; Mediavilla, A.; Pascual, J. P.; Piccirillo, L.; Maffei, B.; Pisano, G.; Watson, R. A.; Davis, R.; Davies, R.; Battye, R.; Saunders, R.; Grainge, K.; Scott, P.; Hobson, M.; Lasenby, A.; Murga, G.; Gomez, C.; Gomez, A.; Arino, J.; Sanquirce, R.; Pan, J.; Vizcarguenaga, A.; Etxeita, B.. - (2010), pp. 127-135. (Intervento presentato al convegno 8th Scientific Meeting of the Spanish Astronomical Society, SEA 2008 tenutosi a Santander, esp) [10.1007/978-3-642-11250-8_12].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1585916
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