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arxiv: 1812.00785 · v4 · pith:PNZR4NVDnew · submitted 2018-11-30 · 🌌 astro-ph.IM

QUBIC: Exploring the primordial Universe with the Q\&U Bolometric Interferometer

Aniello Mennella , Peter Ade , Giorgio Amico , Didier Auguste , Jonathan Aumont , Stefano Banfi , Gustavo Barbar\`an , Paola Battaglia
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Elia Battistelli Alessandro Ba\`u Benoit B\'elier David G. Bennett Laurent Berg\'e Jean Philippe Bernard Marco Bersanelli Marie Anne Bigot Sazy Nathat Bleurvacq Juan Bonaparte Julien Bonis Emory F. Bunn David Burke Daniele Buzi Alessandro Buzzelli Francesco Cavaliere Pierre Chanial Claude Chapron Romain Charlassier Fabio Columbro Gabriele Coppi Alessandro Coppolecchia Rocco D'Agostino Giuseppe D'Alessandro Paolo De Bernardis Giancarlo De Gasperis Michele De Leo Marco De Petris Andres Di Donato Louis Dumoulin Alberto Etchegoyen Adri\'an Fasciszewski Cristian Franceschet Martin Miguel Gamboa Lerena Beatriz Garcia Xavier Garrido Michel Gaspard Amanda Gault Donnacha Gayer Massimo Gervasi Martin Giard Yannick Giraud H\'eraud Mariano G\'omez Berisso Manuel Gonz\'alez Marcin Gradziel Laurent Grandsire Eric Guerard Jean Christophe Hamilton Diego Harari Vic Haynes Sophie Henrot Versill\'e Duc Thuong Hoang Nicolas Holtzer Federico Incardona Eric Jules Jean Kaplan Andrei Korotkov Christian Kristukat Luca Lamagna Soutiris Loucatos Amy Lowitz Vladimir Lukovic Louis Thibault Ra\`ul Horacio Luterstein Bruno Maffei Stefanos Marnieros Silvia Masi Angelo Mattei Andrew May Mark McCulloch Maria C. Medina Lorenzo Mele Simon J. Melhuish Ludovic Montier Louise Mousset Luis Mariano Mundo John Anthony Murphy James Murphy Creidhe O'Sullivan Emiliano Olivieri Alessandro Paiella Francois Pajot Andrea Passerini Hernan Pastoriza Alessandro Pelosi Camille Perbost Maurizio Perciballi Federico Pezzotta Francesco Piacentini Michel Piat Lucio Piccirillo Giampaolo Pisano Gianluca Polenta Damien Pr\^ele Roberto Puddu Damien Rambaud Pablo Ringegni Gustavo E. Romero Maria Salatino Alessandro Schillaci Claudia G. Sc\'occola Stephen P. Scully Sebastiano Spinelli Michail Stolpovskiy Federico Suarez Guillaume Stankowiak Andrea Tartari Jean Pierre Thermeau Peter Timbie Maurizio Tomasi Steve A. Torchinsky Mathieu Tristram Gregory S. Tucker Carole E. Tucker Sylvain Vanneste Daniele Vigan\`o Nicola Vittorio Fabrice Voisin Robert Watson Francois Wicek Mario Zannoni Antonio Zullo
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keywords qubicwillbolometricduringeffectsfrequencyobserveability
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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 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 in 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.

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