%0 Generic %1 Rubino-Martin2008 %A Rubino-Martin, J. A. %A Rebolo, R. %A Tucci, M. %A Genova-Santos, R. %A Hildebrandt, S. R. %A Hoyland, R. %A Herreros, J. M. %A Gomez-Renasco, F. %A Caraballo, C. Lopez %A Martinez-Gonzalez, E. %A Vielva, P. %A Herranz, D. %A Casas, F. J. %A Artal, E. %A Aja, B. %A de la Fuente, L. %A Cano, J. L. %A Villa, E. %A Mediavilla, A. %A Pascual, J. P. %A Piccirillo, L. %A Maffei, B. %A Pisano, G. %A Watson, R. A. %A Davis, R. %A Davies, R. %A Battye, R. %A Saunders, R. %A Grainge, K. %A Scott, P. %A Hobson, M. %A Lasenby, A. %A Murga, G. %A Gomez, C. %A Gomez, A. %A Arino, J. %A Sanquirce, R. %A Pan, J. %A Vizcarguenaga, A. %A Etxeita, B. %D 2008 %K CMB Polarization %T The Quijote CMB Experiment %U http://arxiv.org/abs/0810.3141 %X 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. Comment: 9 pages, 5 figures. To appear in "Highlights of Spanish Astrophysics V", Proceedings of the VIII Scientific Meeting of the Spanish Astronomical Society (SEA) held in Santander, 7-11 July, 2008. Edited by J. Gorgas, L. J. Goicoechea, J. I. Gonzalez-Serrano, J. M. Diego

@misc{Rubino-Martin2008, abstract = { 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. Comment: 9 pages, 5 figures. To appear in "Highlights of Spanish Astrophysics V", Proceedings of the VIII Scientific Meeting of the Spanish Astronomical Society (SEA) held in Santander, 7-11 July, 2008. Edited by J. Gorgas, L. J. Goicoechea, J. I. Gonzalez-Serrano, J. M. Diego}, added-at = {2009-06-08T16:16:03.000+0200}, author = {Rubino-Martin, J. A. and Rebolo, R. and Tucci, M. and Genova-Santos, R. and Hildebrandt, S. R. and Hoyland, R. and Herreros, J. M. and Gomez-Renasco, F. and Caraballo, C. Lopez and Martinez-Gonzalez, E. and Vielva, P. and Herranz, D. and Casas, F. J. and Artal, E. and Aja, B. and de la Fuente, L. and Cano, J. L. and Villa, E. and Mediavilla, A. and Pascual, J. P. and Piccirillo, L. and Maffei, B. and Pisano, G. and Watson, R. A. and Davis, R. and Davies, R. and Battye, R. and Saunders, R. and Grainge, K. and Scott, P. and Hobson, M. and Lasenby, A. and Murga, G. and Gomez, C. and Gomez, A. and Arino, J. and Sanquirce, R. and Pan, J. and Vizcarguenaga, A. and Etxeita, B.}, biburl = {https://www.bibsonomy.org/bibtex/2d64172c44f7581a7c21493441722b815/ad4}, description = {The Quijote CMB Experiment}, interhash = {a655e8d9ad78952b85d943ba7dc8e6ef}, intrahash = {d64172c44f7581a7c21493441722b815}, keywords = {CMB Polarization}, timestamp = {2009-06-08T16:16:03.000+0200}, title = {{T}he {Q}uijote {CMB} {E}xperiment}, url = {http://arxiv.org/abs/0810.3141}, year = 2008 }