> Detailanzeige
Mennella, Aniello;
Ade, Peter;
Amico, Giorgio;
Auguste, Didier;
Aumont, Jonathan;
Banfi, Stefano;
Barbaràn, Gustavo;
Battaglia, Paola;
Battistelli, Elia;
Baù, Alessandro;
Bélier, Benoit;
Bennett, David;
Bergé, Laurent;
Bernard, Jean;
Bersanelli, Marco;
Bigot Sazy, Marie;
Bleurvacq, Nathan;
Bonaparte, Juan;
Bonis, Julien;
Bunn, Emory;
Burke, David;
Buzi, Daniele;
Buzzelli, Alessandro;
Cavaliere, Francesco;
[...]
QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
Teilen
Literatur-
verwaltung
Direktlink
Zur
Merkliste
Lösche von
Merkliste
Per Email teilen
Auf Twitter teilen
Auf Facebook teilen
Per Whatsapp teilen
- Medientyp: E-Artikel
- Titel: QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer
- Beteiligte: Mennella, Aniello; Ade, Peter; Amico, Giorgio; Auguste, Didier; Aumont, Jonathan; Banfi, Stefano; Barbaràn, Gustavo; Battaglia, Paola; Battistelli, Elia; Baù, Alessandro; Bélier, Benoit; Bennett, David; Bergé, Laurent; Bernard, Jean; Bersanelli, Marco; Bigot Sazy, Marie; Bleurvacq, Nathan; Bonaparte, Juan; Bonis, Julien; Bunn, Emory; Burke, David; Buzi, Daniele; Buzzelli, Alessandro; Cavaliere, Francesco; [...]
- Erschienen: MDPI AG, 2019
- Erschienen in: Universe
- Umfang: 42
- Sprache: Englisch
- DOI: 10.3390/universe5020042
- ISSN: 2218-1997
- Schlagwörter: General Physics and Astronomy
- Zusammenfassung: <jats:p>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.</jats:p>
- Beschreibung: <jats:p>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.</jats:p>
- Anmerkungen:
- Zugangsstatus: Freier Zugang