Zobrazeno 1 - 10
of 166
pro vyhledávání: '"Cano, J. L."'
Autor:
Poidevin, F., Rubino-Martin, J. A., Genova-Santos, R., Rebolo, R., Aguiar, M., Gomez-Renasco, F., Guidi., F., Gutierrez, C., Hoyland, R. J., Lopez-Caraballo, C., Carreras, A. Oria, Pelaez-Santos, A. E., Perez-De-Taoro, M. R., Ruiz-Granados, B., Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignaga, R., Martinez-Gonzalez, E., Barreiro, R. B., Casaponsa, B., Casas, F. J., Diego, J. M., Fernandez-Cobos, R., Herranz, D., Lopez-Caniego, M., Ortiz, D., Vielva, P., Artal, E., Aja, B., Cagigas, J., Cano, J. L., De La Fuente, L., Mediavilla, A., Teran, J. V., Villa, E., Piccirillo, L., Dickinson, C., Grainge, K., Harper, S., Mcculloch, M., Melhuish, S., Pisano, G., Watson, R. A., Lasenby, A., Ashdown, M., Perrott, Y., Razavi-Ghods, N., Titterington, D., Scott, P.
Publikováno v:
Proceeding of the 13th Rencontres du Vietnam, July 9-15, 2017, ICISE, Quy Nhon, Vietnam
QUIJOTE (Q-U-I JOint TEnerife) is an experiment designed to achieve CMB B-mode polarization detection and sensitive enough to detect a primordial gravitational-wave component if the B-mode amplitude is larger than r = 0.05. It consists in two telesco
Externí odkaz:
http://arxiv.org/abs/1802.04594
Autor:
Génova-Santos, R., Rubiño-Martín, J. A., Rebolo, R., Aguiar, M., Gómez-Reñasco, F., Gutiérrez, C., Hoyland, R. J., López-Caraballo, C., Peláez-Santos, A. E., de Taoro, M. R. Pérez, Poidevin, F., de la Rosa, V. Sánchez, Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignaga, R., Martínez-González, E., Barreiro, R. B., Casaponsa, 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., Davies, Davis, R. J., Dickinson, C., Grainge, K., Harper, S., Maffei, B., McCulloch, M., Melhuish, S., Pisano, G., Watson, R. A., Lasenby, A., Ashdown, M., Hobson, M., Perrott, Y., Razavi-Ghods, N., Saunders, R., Titterington, D., Scott, P.
QUIJOTE (Q-U-I JOint TEnerife) is a new polarimeter aimed to characterize the polarization of the Cosmic Microwave Background and other Galactic and extragalactic signals at medium and large angular scales in the frequency range 10-40 GHz. The multi-
Externí odkaz:
http://arxiv.org/abs/1504.03514
Autor:
López-Caniego, M., Rebolo, R., Aguiar, M., Génova-Santos, R., Gómez-Reñasco, F., Gutierrez, C., Herreros, J. M., Hoyland, R. J., López-Caraballo, C., Santos, A. E. Pelaez, Poidevin, F., Rubiño-Martín, J. A., de la Rosa, V. Sanchez, Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignaga, R., Martínez-González, E., Barreiro, R. B., Casaponsa, B., Casas, F. J., Diego, J. M., Fernández-Cobos, R., Herranz, D., 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., Grainge, K., Harper, S., Maffei, B., McCulloch, M., Melhuish, S., Pisano, G., Watson, R. A., Hobson, M., Lasenby, A., Saunders, R., Scott, P.
The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment is designed to observe the polarization of the Cosmic Microwave Background and other Galactic and extragalactic signals at medium and large angular scales in the frequency range of 10-40 GHz. The firs
Externí odkaz:
http://arxiv.org/abs/1401.4690
Autor:
Rubino-Martin, J. A., Rebolo, R., Tucci, M., Genova-Santos, R., Hildebrandt, S. R., Hoyland, R., Herreros, J. M., Gomez-Renasco, F., Caraballo, C. Lopez, Martinez-Gonzalez, E., Vielva, P., Herranz, D., Casas, F. J., Artal, E., Aja, B., de la 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.
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 galact
Externí odkaz:
http://arxiv.org/abs/0810.3141
Akademický článek
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Autor:
Engel, K., Pugliatti, Mattia, Drube, Line, Hestroffer, Daniel, Cano, J. L., Delchambre, Simon, Ziegler, Tobias, Johann, Ulrich, Harris, Alan
Near Earth Object (NEO) deflection for the purpose of Earth impact prevention is recognized as a valid and valuable endeavour. NEOTωIST stands for Near-Earth Object Transfer of angular momentum (ω) Spin Test. This describes a demonstration mission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1640::a86b5b8ec579def1de161f9cc470a89a
https://elib.dlr.de/111689/
https://elib.dlr.de/111689/
Autor:
Molina-Cano, J.-L.1 joseluis.molina@irta.es, Moralejo, M.1, Elía, M.1, Muñoz, P.1, Russell, J. R.2, Pérez-Vendrell, A. M.3, Ciudad, F.4, Swanston, J. S.2
Publikováno v:
Molecular Breeding. Apr2007, Vol. 19 Issue 3, p275-284. 10p. 1 Chart, 2 Graphs.
Autor:
Rubiño-Martín, J. A., Génova-Santos, R., Rebolo, R., Aguiar, M., Juan Cozar-Castellano, Gómez-Reñasco, F., Gutiérrez, C., Hoyland, R. J., López-Caraballo, C., Peláez-Santos, A. E., Pérez-De-Taoro, M. R., Poidevin, F., Ruiz-Granados, B., Sánchez La Rosa, V., Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignaga, R., Martínez-González, E., Barreiro, R. B., Casaponsa, 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., La Fuente, L., Mediavilla, A., Terán, J. V., Villa, E., Piccirillo, L., Dickinson, C., Grainge, K., Harper, S., Maffei, B., Mcculloch, M., Melhuish, S., Pisano, G., Watson, R. A., Lasenby, A., Ashdown, M., Perrott, Y., Razavi-Ghods, N., Titterington, D., Scott, P.
Publikováno v:
Highlights on Spanish Astrophysics IX: Proceedings of the XII Scientific Meeting of the Spanish Astronomical Society held on July 18 – 22, 2016, in Bilbao, Spain
Scopus-Elsevier
Scopus-Elsevier
We present the current status of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a new polarimeter with the aim of characterizing the polarization of the Cosmic Microwave Background, and other galactic or extra-galactic physical processes that emit in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3abfb1fe3acc8d2999f511510f76aee2
Autor:
Drube, Line, Harris, Alan W., Schwartz, S., Michel, Patrick, Falke, A., Engel, Kilian, Johann, Ulrich, Eggl, S., Cano, J. L., Martín Ávila, Javier
We present a concept for a kinetic impactor demonstration mission, which aims to change the spin rate of an asteroid. The mission would determine the efficiency of momentum transfer during an impact, and help mature the technology required for a kine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1640::77b76e32189d45b34e84e76e7ac4a866
https://elib.dlr.de/100045/
https://elib.dlr.de/100045/
Autor:
Génova-Santos, R., Rubiño-Martín, J. A., Rebolo, R., Aguiar, M., Gómez-Reñasco, F., Gutiérrez, C., Hoyland, R. J., López-Caraballo, C., Peláez-Santos, A. E., Pérez-De-Taoro, M. R., Poidevin, F., Sánchez La Rosa, V., Tramonte, D., Vega-Moreno, A., Viera-Curbelo, T., Vignasa, R., Martínez-González, E., Barreiro, R. B., Casaponsa, 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., La Fuente, L., Mediavilla, A., Terán, J. V., Villa, E., Piccirillo, L., Davies, R., Davis, R. J., Dickinson, C., Grainge, K., Harper, S., Maffei, B., Mcculloch, M., Melhuish, S., Pisano, G., Robert Watson, Lasenby, A., Ashdown, M., Hobson, M., Perrott, Y., Razavi-Ghods, N., Saunders, R., Titterington, D., Scott, P.
Publikováno v:
Scopus-Elsevier
University of Manchester-PURE
NASA Astrophysics Data System
University of Manchester-PURE
NASA Astrophysics Data System
QUIJOTE (Q-U-I JOint TEnerife) is a new polarimeter aimed to characterize the polarization of the Cosmic Microwave Background and other Galactic and extragalactic signals at medium and large angular scales in the frequency range 10-40 GHz. The multi-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2d58e1cbeb38138a8dc4a30cfe3bc8c
http://hdl.handle.net/11573/1585920
http://hdl.handle.net/11573/1585920