activity
20032022
most citedPlanck pre-launch status: Design and description of the Low Frequency Instrument

176 citations · 357 across the 10 of their papers we have counts for

collaborators

10 papers

hep-ex2022★ 46 cited

The Canfranc Axion Detection Experiment (CADEx): Search for axions at 90 GHz with Kinetic Inductance Detectors

Beatriz Aja, Sergio Arguedas Cuendis, Ivan Arregui +33

We propose a novel experiment, the Canfranc Axion Detection Experiment (CADEx), to probe dark matter axions with masses in the range 330-460 eV, within the W-band (80-110 GHz),…

astro-ph.CO2018★ 8 cited

The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization

F. Poidevin, J. A. Rubino-Martin, R. Genova-Santos +47

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 th…

astro-ph.CO2015★ 15 cited

The QUIJOTE experiment: project overview and first results

R. Génova-Santos, J. A. Rubiño-Martín, R. Rebolo +50

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…

astro-ph.IM2014★ 9 cited

The QUIJOTE CMB Experiment: status and first results with the multi-frequency instrument

M. López-Caniego, R. Rebolo, M. Aguiar +49

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…

astro-ph.IM2010★ 13 cited

Planck pre-launch status: calibration of the Low Frequency Instrument flight model radiometers

F. Villa, L. Terenzi, M. Sandri +71

The Low Frequency Instrument (LFI) on-board the ESA Planck satellite carries eleven radiometer subsystems, called Radiometer Chain Assemblies (RCAs), each composed of a pair of pse…

astro-ph.IM2010★ 16 cited

LFI 30 and 44 GHz receivers Back-End Modules

E. Artal, B. Aja, M. L. de la Fuente +19

The 30 and 44 GHz Back End Modules (BEM) for the Planck Low Frequency Instrument are broadband receivers (20% relative bandwidth) working at room temperature. The signals coming fr…