@conference{10902/38422,
year = {2013},
url = {https://hdl.handle.net/10902/38422},
abstract = {A comparison between simulated and measured results in different subsystems of a radio astronomy polarimeter receiver at 26–36 GHz band is presented. This comparison underlines the importance of careful simulation with different electromagnetic software tools in order to predict the receiver behavior. The receiver obtains three (Q, U and I) Stokes parameters simultaneously.},
organization = {This work has been funded by the Ministerio de Ciencia e Innovación (Spain) under Astronomy and Astrophysics research programme, reference AYA2010–21766-C03–03.},
publisher = {Institute of Electrical and Electronics Engineers, Inc.},
publisher = {International Conference on Electromagnetics in Advanced Applications (ICEAA), Torino, Italy, 2013, 250-253},
title = {EM developments for a radio astronomy polarimeter: The QUIJOTE experiment},
author = {Artal Latorre, Eduardo and Cano de Diego, Juan Luis and Mediavilla Sánchez, Ángel and Villa Benito, Enrique and Aja Abelán, Beatriz and Fuente Rodríguez, Luisa María de la and Cagigas Ibañez, Jaime},
}