BibSonomyburst/author/Lopez CaraballoBibSonomy RSS feed for /author/Lopez Caraballo2012-02-16T16:42:08+01:00http://www.bibsonomy.org/bibtex/2d64172c44f7581a7c21493441722b815/ptomicoptomico2009-12-23T22:19:09+01:00cmb experiment quijote <span class="authorEditorList"><a href="/author/Rubino-Martin">J. A. Rubino-Martin</a>, <a href="/author/Rebolo">R. Rebolo</a>, <a href="/author/Tucci">M. Tucci</a>, <a href="/author/Genova-Santos">R. Genova-Santos</a>, <a href="/author/Hildebrandt">S. R. Hildebrandt</a>, <a href="/author/Hoyland">R. Hoyland</a>, <a href="/author/Herreros">J. M. Herreros</a>, <a href="/author/Gomez-Renasco">F. Gomez-Renasco</a>, <a href="/author/Caraballo">C. Lopez Caraballo</a>, <a href="/author/Martinez-Gonzalez">E. Martinez-Gonzalez</a>, <a href="/author/Vielva">P. Vielva</a>, <a href="/author/Herranz">D. Herranz</a>, <a href="/author/Casas">F. J. Casas</a>, <a href="/author/Artal">E. Artal</a>, <a href="/author/Aja">B. Aja</a>, <a href="/author/de la Fuente">L. de la Fuente</a>, <a href="/author/Cano">J. L. Cano</a>, <a href="/author/Villa">E. Villa</a>, <a href="/author/Mediavilla">A. Mediavilla</a>, <a href="/author/Pascual">J. P. Pascual</a>, <a href="/author/Piccirillo">L. Piccirillo</a>, <a href="/author/Maffei">B. Maffei</a>, <a href="/author/Pisano">G. Pisano</a>, <a href="/author/Watson">R. A. Watson</a>, <a href="/author/Davis">R. Davis</a>, <a href="/author/Davies">R. Davies</a>, <a href="/author/Battye">R. Battye</a>, <a href="/author/Saunders">R. Saunders</a>, <a href="/author/Grainge">K. Grainge</a>, <a href="/author/Scott">P. Scott</a>, <a href="/author/Hobson">M. Hobson</a>, <a href="/author/Lasenby">A. Lasenby</a>, <a href="/author/Murga">G. Murga</a>, <a href="/author/Gomez">C. Gomez</a>, <a href="/author/Gomez">A. Gomez</a>, <a href="/author/Arino">J. Arino</a>, <a href="/author/Sanquirce">R. Sanquirce</a>, <a href="/author/Pan">J. Pan</a>, <a href="/author/Vizcarguenaga">A. Vizcarguenaga</a>, and <a href="/author/Etxeita">B. Etxeita</a> </span>(<em>2008</em>)Wed Dec 23 22:19:09 CET 2009{T}he {Q}uijote {CMB} {E}xperiment2008cmb experiment quijote 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 &quot;Highlights of Spanish Astrophysics V&quot;, 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. DiegoThe Quijote CMB Experimenthttp://www.bibsonomy.org/bibtex/2d64172c44f7581a7c21493441722b815/ad4ad42009-06-08T16:16:03+02:00CMB Polarization <span class="authorEditorList"><a href="/author/Rubino-Martin">J. A. Rubino-Martin</a>, <a href="/author/Rebolo">R. Rebolo</a>, <a href="/author/Tucci">M. Tucci</a>, <a href="/author/Genova-Santos">R. Genova-Santos</a>, <a href="/author/Hildebrandt">S. R. Hildebrandt</a>, <a href="/author/Hoyland">R. Hoyland</a>, <a href="/author/Herreros">J. M. Herreros</a>, <a href="/author/Gomez-Renasco">F. Gomez-Renasco</a>, <a href="/author/Caraballo">C. Lopez Caraballo</a>, <a href="/author/Martinez-Gonzalez">E. Martinez-Gonzalez</a>, <a href="/author/Vielva">P. Vielva</a>, <a href="/author/Herranz">D. Herranz</a>, <a href="/author/Casas">F. J. Casas</a>, <a href="/author/Artal">E. Artal</a>, <a href="/author/Aja">B. Aja</a>, <a href="/author/de la Fuente">L. de la Fuente</a>, <a href="/author/Cano">J. L. Cano</a>, <a href="/author/Villa">E. Villa</a>, <a href="/author/Mediavilla">A. Mediavilla</a>, <a href="/author/Pascual">J. P. Pascual</a>, <a href="/author/Piccirillo">L. Piccirillo</a>, <a href="/author/Maffei">B. Maffei</a>, <a href="/author/Pisano">G. Pisano</a>, <a href="/author/Watson">R. A. Watson</a>, <a href="/author/Davis">R. Davis</a>, <a href="/author/Davies">R. Davies</a>, <a href="/author/Battye">R. Battye</a>, <a href="/author/Saunders">R. Saunders</a>, <a href="/author/Grainge">K. Grainge</a>, <a href="/author/Scott">P. Scott</a>, <a href="/author/Hobson">M. Hobson</a>, <a href="/author/Lasenby">A. Lasenby</a>, <a href="/author/Murga">G. Murga</a>, <a href="/author/Gomez">C. Gomez</a>, <a href="/author/Gomez">A. Gomez</a>, <a href="/author/Arino">J. Arino</a>, <a href="/author/Sanquirce">R. Sanquirce</a>, <a href="/author/Pan">J. Pan</a>, <a href="/author/Vizcarguenaga">A. Vizcarguenaga</a>, and <a href="/author/Etxeita">B. Etxeita</a> </span>(<em>2008</em>)Mon Jun 08 16:16:03 CEST 2009{T}he {Q}uijote {CMB} {E}xperiment2008CMB Polarization 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 &quot;Highlights of Spanish Astrophysics V&quot;, 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. DiegoThe Quijote CMB Experiment