QUBIC II: Spectral polarimetry with bolometric interferometry
dc.contributor.author | Mousset, L. | |
dc.contributor.author | Lerena, M. M. Gamboa | |
dc.contributor.author | Battistelli, E. S. | |
dc.contributor.author | de Bernardis, P. | |
dc.contributor.author | Chanial, P. | |
dc.contributor.author | D'Alessandro, G. | |
dc.contributor.author | Dashyan, G. | |
dc.contributor.author | De Petris, M. | |
dc.contributor.author | Grandsire, L. | |
dc.contributor.author | Hamilton, J. -Ch. | |
dc.contributor.author | Incardona, F. | |
dc.contributor.author | Landau, S. | |
dc.contributor.author | Marnieros, S. | |
dc.contributor.author | Masi, S. | |
dc.contributor.author | Mennella, A. | |
dc.contributor.author | O'Sullivan, C. | |
dc.contributor.author | Piat, M. | |
dc.contributor.author | Ricciardi, G. | |
dc.contributor.author | Scoccola, C. G. | |
dc.contributor.author | Stolpovskiy, M. | |
dc.contributor.author | Tartari, A. | |
dc.contributor.author | Thermeau, J. -P. | |
dc.contributor.author | Torchinsky, S. A. | |
dc.contributor.author | Voisin, F. | |
dc.contributor.author | Zannoni, M. | |
dc.contributor.author | Ade, P. | |
dc.contributor.author | Alberro, J. G. | |
dc.contributor.author | Almela, A. | |
dc.contributor.author | Amico, G. | |
dc.contributor.author | Arnaldi, L. H. | |
dc.contributor.author | Auguste, D. | |
dc.contributor.author | Aumont, J. | |
dc.contributor.author | Azzoni, S. | |
dc.contributor.author | Banfi, S. | |
dc.contributor.author | Bau, A. | |
dc.contributor.author | Belier, B. | |
dc.contributor.author | Bennett, D. | |
dc.contributor.author | Berge, L. | |
dc.contributor.author | Bernard, J. -Ph. | |
dc.contributor.author | Bersanelli, M. | |
dc.contributor.author | Bigot-Sazy, M. -A. | |
dc.contributor.author | Bonaparte, J. | |
dc.contributor.author | Bonis, J. | |
dc.contributor.author | Bunn, E. | |
dc.contributor.author | Burke, D. | |
dc.contributor.author | Buzi, D. | |
dc.contributor.author | Cavaliere, F. | |
dc.contributor.author | Chapron, C. | |
dc.contributor.author | Charlassier, R. | |
dc.contributor.author | Cerutti, A. C. Cobos | |
dc.contributor.author | Columbro, F. | |
dc.contributor.author | Coppolecchia, A. | |
dc.contributor.author | De Gasperis, G. | |
dc.contributor.author | De Leo, M. | |
dc.contributor.author | Dheilly, S. | |
dc.contributor.author | Duca, C. | |
dc.contributor.author | Dumoulin, L. | |
dc.contributor.author | Etchegoyen, A. | |
dc.contributor.author | Fasciszewski, A. | |
dc.contributor.author | Ferreyro, L. P. | |
dc.contributor.author | Fracchia, D. | |
dc.contributor.author | Franceschet, C. | |
dc.contributor.author | Ganga, K. M. | |
dc.contributor.author | Garcia, B. | |
dc.contributor.author | Redondo, M. E. Garcia | |
dc.contributor.author | Gaspard, M. | |
dc.contributor.author | Gayer, D. | |
dc.contributor.author | Gervasi, M. | |
dc.contributor.author | Giard, M. | |
dc.contributor.author | Gilles, V. | |
dc.contributor.author | Giraud-Heraud, Y. | |
dc.contributor.author | Berisso, M. Gomez | |
dc.contributor.author | Gonzalez, M. | |
dc.contributor.author | Gradziel, M. | |
dc.contributor.author | Hampel, M. R. | |
dc.contributor.author | Harari, D. | |
dc.contributor.author | Henrot-Versille, S. | |
dc.contributor.author | Jules, E. | |
dc.contributor.author | Kaplan, J. | |
dc.contributor.author | Kristukat, C. | |
dc.contributor.author | Lamagna, L. | |
dc.contributor.author | Loucatos, S. | |
dc.contributor.author | Louis, T. | |
dc.contributor.author | Maffei, B. | |
dc.contributor.author | Mandelli, S. | |
dc.contributor.author | Marty, W. | |
dc.contributor.author | Mattei, A. | |
dc.contributor.author | May, A. | |
dc.contributor.author | McCulloch, M. | |
dc.contributor.author | Mele, L. | |
dc.contributor.author | Melo, D. | |
dc.contributor.author | Montier, L. | |
dc.contributor.author | Mundo, L. M. | |
dc.contributor.author | Murphy, J. A. | |
dc.contributor.author | Murphy, J. D. | |
dc.contributor.author | Nati, F. | |
dc.contributor.author | Olivieri, E. | |
dc.contributor.author | Oriol, C. | |
dc.contributor.author | Paiella, A. | |
dc.contributor.author | Pajot, F. | |
dc.contributor.author | Passerini, A. | |
dc.contributor.author | Pastoriza, H. | |
dc.contributor.author | Pelosi, A. | |
dc.contributor.author | Perbost, C. | |
dc.contributor.author | Perciballi, M. | |
dc.contributor.author | Pezzotta, F. | |
dc.contributor.author | Piacentini, F. | |
dc.contributor.author | Piccirillo, L. | |
dc.contributor.author | Pisano, G. | |
dc.contributor.author | Platino, M. | |
dc.contributor.author | Polenta, G. | |
dc.contributor.author | Prele, D. | |
dc.contributor.author | Puddu, R. | |
dc.contributor.author | Rambaud, D. | |
dc.contributor.author | Rasztocky, E. | |
dc.contributor.author | Ringegni, P. | |
dc.contributor.author | Romero, G. E. | |
dc.contributor.author | Salum, J. M. | |
dc.contributor.author | Schilaci, A. | |
dc.contributor.author | Scully, S. | |
dc.contributor.author | Spinelli, S. | |
dc.contributor.author | Stankowiak, G. | |
dc.contributor.author | Supanitsky, A. D. | |
dc.contributor.author | Timbie, P. | |
dc.contributor.author | Tomasi, M. | |
dc.contributor.author | Tucker, C. | |
dc.contributor.author | Tucker, G. | |
dc.contributor.author | Vigano, D. | |
dc.contributor.author | Vittorio, N. | |
dc.contributor.author | Wicek, F. | |
dc.contributor.author | Wright, M. | |
dc.contributor.author | Zullo, A. | |
dc.date.accessioned | 2025-01-20T21:03:01Z | |
dc.date.available | 2025-01-20T21:03:01Z | |
dc.date.issued | 2022 | |
dc.description.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 mi-crowave 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-mo de polarization of the sky at millimeter wavelengths. We consider the specific cases of point source reconstruc-tion 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. | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.1088/1475-7516/2022/04/035 | |
dc.identifier.issn | 1475-7516 | |
dc.identifier.uri | https://doi.org/10.1088/1475-7516/2022/04/035 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/93114 | |
dc.identifier.wosid | WOS:000807377200005 | |
dc.issue.numero | 4 | |
dc.language.iso | en | |
dc.revista | Journal of cosmology and astroparticle physics | |
dc.rights | acceso restringido | |
dc.subject | CMBR experiments | |
dc.subject | CMBR theory | |
dc.subject | cosmological parameters from CMBR | |
dc.subject | grav-itational waves and CMBR polarization | |
dc.title | QUBIC II: Spectral polarimetry with bolometric interferometry | |
dc.type | artículo | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |