activity
20032018
most citedPlanck pre-launch status: Low Frequency Instrument calibration and expected scientific performance

43 citations · 99 across the 6 of their papers we have counts for

collaborators

6 papers

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★ 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…

astro-ph.IM2010★ 43 cited

Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance

A. Mennella, M. Bersanelli, R. C. Butler +83

We give the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters char…

astro-ph2003★ 8 cited

Advanced pseudo-correlation radiometers for the Planck-LFI instrument

A. Mennella, M. Bersanelli, R. C. Butler +34

The LFI (Low Frequency Instrument) on board the ESA Planck satellite is constituted by an array of radiometric detectors actively cooled at 20 K in the 30-70 GHz frequency range in…