Mennella, Aniello, Ade, Peter ![]() ![]() ![]() ![]() ![]() |
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Abstract
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.
Item Type: | Article |
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Date Type: | Published Online |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | MDPI |
ISSN: | 2218-1997 |
Date of First Compliant Deposit: | 12 March 2019 |
Date of Acceptance: | 16 January 2019 |
Last Modified: | 09 Oct 2023 20:00 |
URI: | https://orca.cardiff.ac.uk/id/eprint/120565 |
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