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The Quijote CMB Experiment

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arxiv 0810.3141 v1 pith:QTCWWTWU submitted 2008-10-17 astro-ph

The Quijote CMB Experiment

J.A. Rubino-Martin , R. Rebolo , M. Tucci , R. Genova-Santos , S.R. Hildebrandt , R. Hoyland , J.M. Herreros , F. Gomez-Renasco
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C. Lopez Caraballo E. Martinez-Gonzalez P. Vielva D. Herranz F.J. Casas E. Artal B. Aja L. de la Fuente J.L. Cano E. Villa A. Mediavilla J.P. Pascual L. Piccirillo B. Maffei G. Pisano R.A. Watson R. Davis R. Davies R. Battye R. Saunders K. Grainge P. Scott M. Hobson A. Lasenby G. Murga C. Gomez A. Gomez J. Arino R. Sanquirce J. Pan A. Vizcarguenaga B. Etxeita
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keywords quijotewillexperimentangularcharacterizingcomplementcomponentcurrent
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We present the current status of the QUIJOTE (Q-U-I JOint TEnerife) CMB Experiment, a new instrument which will start operations early 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 10-30 GHz 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=0.05.

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