M. Aguiar

Computational Solutions for Supporting Systematic Reviews in Software Engineering: a Comprehensive Overview

M. Aguiar, Érica Ferreira de Souza, Katia Romero Felizardo, Luciana Brasil Rebelo dos Santos

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Yellow Fever Virus Induces Golgi Stress and CREB3L1 Nuclear Translocation in Human A549 Cells

María Florencia Ferrer, Victoria Rozés‐Salvador, Carla Tomatis, Pablo Javier Thomas et autres

Yellow fever is an endemic disease in Africa and South America caused by the homonymous flavivirus (YFV). The disease can manifest as a febrile syndrome and, in the most severe cases, liver failure and death. Although it can be prevented by a …

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The role of bioremediation in mitigating urban expansion impacts on coastal lagoons: A comparative study of Araçatiba and Padre Lagoons, Rio de Janeiro

Renan M. Amorim, L W Gaudie-Ley, M. Aguiar, P da S Sant'Anna et autres

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KISS: Instrument Description and Performance

Juan Francisco Macias-Perez, M Fernández-Torreiro, A. Catalano, A. Fasano et autres

Abstract Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimeter range. Their compact size enables them to optimally fill the focal plane, thus boosting sensitivity. The KIDs Interferometric Spectral Surveyor (KISS) instrument is a …

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KISS: instrument description and performance

J. -F. Macías-Pérez, M Fernández-Torreiro, A. Catalano, Alessio Fasano et autres

Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimetre range. Their compact size enables to optimally fill the focal plane, thus boosting sensitivity. The KISS (KIDs Interferometric Spectral Surveyor) instrument is a millimetre camera …

fr (code pays fourni par la source)

Observations with KIDs Interferometer Spectrum Survey (KISS)

A. Fasano, A. Catalano, Juan Francisco Macias-Perez, M. Aguiar et autres

We describe the preliminary on-sky results of the KIDs Interferometer Spectrum Survey (KISS), a spectral imager with a 1 deg field of view (FoV). The instrument operates in the range 120–180 GHz from the 2.25m Q-U-I JOint TEnerife telescope in Teide Observatory …

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Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors

A. Fasano, Juan Francisco Macias-Perez, A. Benoı̂t, M. Aguiar et autres

Context.Wide-field spectrometers are needed to deal with current astrophysical challenges that require multiband observations at millimeter wavelengths. An example of these is the KIDs Interferometer Spectrum Survey (KISS), which uses two arrays of kinetic inductance detectors (KIDs) coupled to a Martin-Puplett interferometer …

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The KISS Experiment

A. Fasano, M. Aguiar, A. Benoı̂t, A. Bideaud et autres

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

Frédérick Poidevin, José Alberto Rubiño-Martín, Ricardo Tanausú Génova-Santos, Rafael Rebolo et autres

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 telescopes and three instruments observing …

The QUIJOTE experiment: project status and first scientific results

José Alberto Rubiño-Martín, Ricardo Tanausú Génova-Santos, Rafael Rebolo, M. Aguiar et autres

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 microwaves in the frequency range …

The QUIJOTE experiment: project overview and first results

R. T. Génova-Santos, José Alberto Rubiño-Martín, Rafael Rebolo, M. Aguiar et autres

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-frequency (10-20~GHz) instrument, mounted on …

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

M. López-Caniego, Rafael Rebolo, M. Aguiar, R. T. Génova-Santos et autres

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 first of the two …