QUBIC II: Spectral polarimetry with bolometric interferometry. Issue 4 (1st April 2022)

• Record Type: Journal Article
• Authors: Mousset, L.; Gamboa Lerena, M.M.; Battistelli, E.S.; de Bernardis, P.; Chanial, P.; D'Alessandro, G.; Dashyan, G.; De Petris, M.; Grandsire, L.; Hamilton, J.-Ch.; Incardona, F.; Landau, S.; Marnieros, S.; Masi, S.; Mennella, A.; O'Sullivan, C.; Piat, M.; Ricciardi, G.; Scóccola, C.G.; Stolpovskiy, M.; Tartari, A.; Thermeau, J.-P.; Torchinsky, S.A.; Voisin, F.; Zannoni, M.; Ade, P.; Alberro, J.G.; Almela, A.; Amico, G.; Arnaldi, L.H.; Auguste, D.; Aumont, J.; Azzoni, S.; Banfi, S.; Baù, A.; Bélier, B.; Bennett, D.; Bergé, L.; Bernard, J.-Ph.; Bersanelli, M.; Bigot-Sazy, M.-A.; Bonaparte, J.; Bonis, J.; Bunn, E.; Burke, D.; Buzi, D.; Cavaliere, F.; Chapron, C.; Charlassier, R.; Cobos Cerutti, A.C.; Columbro, F.; Coppolecchia, A.; De Gasperis, G.; De Leo, M.; Dheilly, S.; Duca, C.; Dumoulin, L.; Etchegoyen, A.; Fasciszewski, A.; Ferreyro, L.P.; Fracchia, D.; Franceschet, C.; Ganga, K.M.; García, B.; García Redondo, M.E.; Gaspard, M.; Gayer, D.; Gervasi, M.; Giard, M.; Gilles, V.; Giraud-Heraud, Y.; Gómez Berisso, M.; González, M.; Gradziel, M.; Hampel, M.R.; Harari, D.; Henrot-Versillé, S.; Jules, E.; Kaplan, J.; Kristukat, C.; Lamagna, L.; Loucatos, S.; Louis, T.; Maffei, B.; Mandelli, S.; Marty, W.; Mattei, A.; May, A.; McCulloch, M.; Mele, L.; Melo, D.; Montier, L.; Mundo, L.M.; Murphy, J.A.; Murphy, J.D.; Nati, F.; Olivieri, E.; Oriol, C.; Paiella, A.; Pajot, F.; Passerini, A.; Pastoriza, H.; Pelosi, A.; Perbost, C.; Perciballi, M.; Pezzotta, F.; Piacentini, F.; Piccirillo, L.; Pisano, G.; Platino, M.; Polenta, G.; Prêle, D.; Puddu, R.; Rambaud, D.; Rasztocky, E.; Ringegni, P.; Romero, G.E.; Salum, J.M.; Schillaci, A.; Scully, S.; Spinelli, S.; Stankowiak, G.; Supanitsky, A.D.; Timbie, P.; Tomasi, M.; Tucker, C.; Tucker, G.; Viganò, D.; Vittorio, N.; Wicek, F.; Wright, M.; Zullo, A.;
• Is Part Of: Journal of cosmology and astroparticle physics. Volume 2022:Issue 4(2022)
• Publication Date: 2022-04-01
• Subjects: CMBR experiments -- CMBR theory -- cosmological parameters from CMBR -- gravitational waves and CMBR polarization; Cosmology -- Periodicals; Astrophysics -- Periodicals; 523.0105
• DOI: 10.1088/1475-7516/2022/04/035
• Languages: English
• ISSNs: 1475-7516

Abstract

Abstract: Bolometric interferometry is a novel technique that has the ability to perform spectral imaging. A bolometric interferometer observes the sky in a wide frequency band and can reconstruct sky maps in several sub-bands within the physical band in post-processing of the data. This provides a powerful spectral method to discriminate between the cosmic microwave background (CMB) and astrophysical foregrounds. In this paper, the methodology is illustrated with examples based on the Q & U Bolometric Interferometer for Cosmology (QUBIC) which is a ground-based instrument designed to measure the B-mode polarization of the sky at millimeter wavelengths. We consider the specific cases of point source reconstruction and Galactic dust mapping and we characterize the point spread function as a function of frequency. We study the noise properties of spectral imaging, especially the correlations between sub-bands, using end-to-end simulations together with a fast noise simulator. We conclude showing that spectral imaging performance are nearly optimal up to five sub-bands in the case of QUBIC.