QUBIC: Exploring the primordial universe with the Q&U bolometric interferometer

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...

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Detalles Bibliográficos
Autores: Mennella, Aniello, Ade, Peter, Amico, Giorgio, Auguste, Didier, Aumont, Jonathan, Banfi, Stefano, Barban, Gustavo, Battaglia, Paola, Battistelli, Elia, Baù, Alessandro, Bélier, Benoit, Bergé, Laurent, Bernard, Jean Philippe, Bersanelli, Marco, Sazy, Marie Anne Bigot, Bleurvacq, Nathan, Bonaparte, Juan José, Bonis, Julien, Bunn, Emory, Burke, David, Buzi, Daniele, Buzzelli, Alessandro, Cavaliere, Francesco, Chanial, Pierre, Chapron, Claude, Charlassier, Romain, Columbro, Fabio, Coppi, Gabriele, Coppolecchia, Alessandro, D'Agostino, Rocco, D'Alessandro, Giuseppe, De Bernardis, Paolo, De Gasperis, Giancarlo, De Leo, Michele, De Petris, Marco, Di Donato, Andrés Leonardo, Dumoulin, Louis, Etchegoyen, Alberto, Fasciszewski, Adrián, Franceschet, Cristian, Gamboa Lerena, Martín Miguel, Garcia, Beatriz Alicia, Garrido, Xavier, Gaspard, Michel, Gault, Amanda, Gayer, Donnacha, Gervasi, Massimo, Giard, Martin, Héraud, Yannick Giraud, Gomez Berisso, Mariano, González, Manuel, Gradziel, Marcin, Grandsire, Laurent, Guerard, Eric, Hamilton, Jean Christophe, Harari, Diego Dario, Haynes, Vic, Versillé, Sophie Henrot, Hoang, Duc Thuong, Holtzer, Nicolas, Incardona, Federico, Jules, Eric, Kaplan, Jean, Korotkov, Andrei, Kristukat, Ralf Christian, Lamagna, Luca, Loucatos, Sotiris, Louis, Thibaut, Lowitz, Amy, Lukovic, Vladimir, Luterstein, Raúl Horacio, Maffei, Bruno, Marnieros, Stefanos, Masi, Silvia, Mattei, Angelo, May, Andrew, McCulloch, Mark, Medina, Maria Clementina, Mele, Lorenzo, Melhuish, Simon J., Montier, Ludovic, Mousset, Louise, Mundo, Luis Mariano, Murphy, John Anthony, Murphy, James David, O'Sullivan, Creidhe, Olivieri, Emiliano, Paiella, Alessandro, Pajot, Francois, Passerini, Andrea, Pastoriza, Hernan, Pelosi, Alessandro, Perbost, Camille, Perciballi, Maurizio, Pezzotta, Federico, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pisano, Giampaolo, Polenta, Gianluca, Prêle, Damien, Puddu, Roberto, Rambaud, Damien, Ringegni, Pablo, Romero, Gustavo Esteban, Salatino, Maria, Schillaci, Alessandro, Scóccola, Claudia G., Scully, Stephen P., Spinelli, Sebastiano, Stankowiak, Guillaume, Stolpovskiy, Michail, Suarez, Federico, Tartari, Andrea, Thermeau, Jean Pierre, Timbie, Peter, Tomasi, Maurizio, Torchinsky, Steve A., Tristram, Matthieu, Tucker, Carole E., Tucker, Gregory S., Vanneste, Sylvain, Viganò, Daniele, Vittorio, Nicola, Voisin, Fabrice, Watson, Robert, Wicek, Francois, Zannoni, Mario, Zullo, Antonio
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:Argentina
Institución:Consejo Nacional de Investigaciones Científicas y Técnicas
Repositorio:CONICET Digital (CONICET)
Idioma:inglés
OAI Identifier:oai:ri.conicet.gov.ar:11336/124008
Acceso en línea:http://hdl.handle.net/11336/124008
Access Level:acceso abierto
Palabra clave:B-MODES
BOLOMETERS
COSMIC MICROWAVE BACKGROUND
INFLATION
POLARIMETRY
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
Descripción
Sumario: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: 150GHz 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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