Zobrazeno 1 - 3
of 3
pro vyhledávání: '"José Alberto Rubiño Martín"'
Autor:
Mateo Fernández-Torreiro, José Alberto Rubiño-Martín, Ricardo Tanausú Génova-Santos, Mike Peel, QUIJOTE collaboration
The Thirty and Forty Gigahertz Instrument (TFGI) observes the sky at 31 and 40 GHz, with ~20 arcminutes resolution. After a first test run during 2018-2019, it was re-mounted on the QUIJOTE experiment (located at the Teide Observatory, Tenerife) on N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::136c379fa507df94aa4d30ff543cfcc0
Autor:
Rafael Toledo-Moreo, Gaizka Murga-Llano, Javier De Miguel-Hernández, Carlos H. López-Caraballo, S. Realini, Federica Guidi, Carlos Colodro-Conde, Jens Chluba, Rafael Rebolo, Ruben Sanquirce-Garcia, C. Hernández-Monteagudo, Michael W. Peel, Paz Alonso Arias, Cristina Perez-Lemus, Antonio Zamora-Jimenez, Eduardo D. González-Carretero, Patricia Fernández-Izquierdo, Pablo A. Fuerte-Rodriguez, Maria F. Gomez-Reñasco, Cristian Franceschet, F. Cuttaia, M. Aguiar-González, Angeles Perez-de-Taoro, Roger J. Hoyland, Ricardo Génova-Santos, David Pérez-Lizán, Luca Terenzi, José Alberto Rubiño Martín, Mateo Fernández-Torreiro
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X.
The Tenerife Microwave Spectrometer (TMS) is a new 10-20 GHz experiment that will be installed at the Teide Observatory (Tenerife, Spain), next to the QUIJOTE CMB experiment. The main TMS scientific driver is to accurately measure absolute distortion
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e7d64074500a60b8110f7184d3e3eb00
https://doi.org/10.1117/12.2561309
https://doi.org/10.1117/12.2561309
Autor:
José Alberto Rubiño-Martín, Antonio M. Aliaga, R. B. Barreiro, Richard A. Battye, Pedro Carreira, Kieran Cleary, Rod D. Davies, Richard J. Davis, Clive Dickinson, Ricardo Génova-Santos, Keith Grainge, Carlos M. Gutiérrez, Yaser A. Hafez, Michael P. Hobson, Michael E. Jones, Rüdiger Kneissl, Katy Lancaster, Anthony Lasenby, J. P. Leahy, Klaus Maisinger, Enrique Martínez-González, Guy G. Pooley, Nutan Rajguru, Rafael Rebolo, José Luis Sanz, Richard D. E. Saunders, Richard S. Savage, Anna Scaife, Paul Scott, Anže Slosar, Angela C. Taylor, David Titterington, Elizabeth Waldram, Robert A. Watson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 369:909-920
We have used the Rayner & Best (1989) smooth tests of goodness-of-fit to studythe Gaussianity of the Very Small Array (VSA) data. These tests are designed to besensitive to the presence of ‘smooth’ deviations from a given distribution, and areap
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06fe7209714799c470859c596cfb0471
https://doi.org/10.1111/j.1365-2966.2006.10341.x
https://doi.org/10.1111/j.1365-2966.2006.10341.x