QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer

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In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self...

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Autores principales: Gamboa Lerena, Martín Miguel, Mundo, Luis Mariano, Ringegni, Pablo Lorenzo, Scóccola, Claudia Graciela
Formato: Articulo
Lenguaje:Inglés
Publicado: 2019
Materias:
Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/124814
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-124814
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
spellingShingle Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
Gamboa Lerena, Martín Miguel
Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
topic_facet Astronomía
B-modes
bolometers
Cosmic Microwave Background
inflation
polarimetry
description In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
format Articulo
Articulo
author Gamboa Lerena, Martín Miguel
Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
author_facet Gamboa Lerena, Martín Miguel
Mundo, Luis Mariano
Ringegni, Pablo Lorenzo
Scóccola, Claudia Graciela
author_sort Gamboa Lerena, Martín Miguel
title QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_short QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_full QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_fullStr QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_full_unstemmed QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
title_sort qubic: exploring the primordial universe with the q&u bolometric interferometer
publishDate 2019
url http://sedici.unlp.edu.ar/handle/10915/124814
work_keys_str_mv AT gamboalerenamartinmiguel qubicexploringtheprimordialuniversewiththequbolometricinterferometer
AT mundoluismariano qubicexploringtheprimordialuniversewiththequbolometricinterferometer
AT ringegnipablolorenzo qubicexploringtheprimordialuniversewiththequbolometricinterferometer
AT scoccolaclaudiagraciela qubicexploringtheprimordialuniversewiththequbolometricinterferometer
bdutipo_str Repositorios
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