QUBIC II: Spectral polarimetry with bolometric interferometry

L. Mousset; M. M. Gamboa Lerena; E. S. Battistelli; P. De Bernardis; P. Chanial; G. D'Alessandro; G. Dashyan; M. De Petris; L. Grandsire; J. Ch Hamilton; F. Incardona; S. Landau; S. Marnieros; S. Masi; A. Mennella; C. O'Sullivan; M. Piat; G. Ricciardi; C. G. Scóccola; M. Stolpovskiy; A. Tartari; J. P. Thermeau; S. A. Torchinsky; F. Voisin; M. Zannoni; P. Ade; J. G. Alberro; A. Almela; G. Amico; L. H. Arnaldi; D. Auguste; J. Aumont; S. Azzoni; S. Banfi; A. Baù; B. Bélier; D. Bennett; L. Bergé; J. Ph Bernard; M. Bersanelli; M. A. Bigot-Sazy; J. Bonaparte; J. Bonis; E. Bunn; D. Burke; D. Buzi; F. Cavaliere; C. Chapron; R. Charlassier; A. C. Cobos Cerutti; F. Columbro; A. Coppolecchia; G. De Gasperis; M. De Leo; S. Dheilly; C. Duca; L. Dumoulin; A. Etchegoyen; A. Fasciszewski; L. P. Ferreyro; D. Fracchia; C. Franceschet; K. M. Ganga; B. García; M. E. García Redondo; M. Gaspard; D. Gayer; M. Gervasi; M. Giard; V. Gilles; Y. Giraud-Heraud; M. Gómez Berisso; M. González; M. Gradziel; M. R. Hampel; D. Harari; S. Henrot-Versillé; E. Jules; J. Kaplan; C. Kristukat; L. Lamagna; S. Loucatos; T. Louis; B. Maffei; S. Mandelli; W. Marty; A. Mattei; A. May; M. McCulloch; L. Mele; D. Melo; L. Montier; L. M. Mundo; J. A. Murphy; F. Nati; E. Olivieri; C. Oriol; A. Paiella; F. Pajot; A. Passerini; H. Pastoriza; A. Pelosi; C. Perbost; M. Perciballi; F. Pezzotta; F. Piacentini; L. Piccirillo; G. Pisano; M. Platino; G. Polenta; D. Prêle; R. Puddu; D. Rambaud; E. Rasztocky; P. Ringegni; G. E. Romero; J. M. Salum; A. Schillaci; S. Scully; S. Spinelli; G. Stankowiak; A. D. Supanitsky; P. Timbie; M. Tomasi; C. Tucker; G. Tucker; D. Viganò; N. Vittorio; F. Wicek; M. Wright; A. Zullo

doi:10.1088/1475-7516/2022/04/035

QUBIC II: Spectral polarimetry with bolometric interferometry

L. Mousset, M. M. Gamboa Lerena, E. S. Battistelli, P. De Bernardis, P. Chanial, G. D'Alessandro, G. Dashyan, M. De Petris, L. Grandsire, J. Ch Hamilton, F. Incardona, S. Landau, S. Marnieros, S. Masi, A. Mennella, C. O'Sullivan, M. Piat, G. Ricciardi, C. G. Scóccola, M. StolpovskiyA. Tartari, J. P. Thermeau, S. A. Torchinsky, F. Voisin, M. Zannoni, P. Ade, J. G. Alberro, A. Almela, G. Amico, L. H. Arnaldi, D. Auguste, J. Aumont, S. Azzoni, S. Banfi, A. Baù, B. Bélier, D. Bennett, L. Bergé, J. Ph Bernard, M. Bersanelli, M. A. Bigot-Sazy, J. Bonaparte, J. Bonis, E. Bunn, D. Burke, D. Buzi, F. Cavaliere, C. Chapron, R. Charlassier, A. C. Cobos Cerutti, F. Columbro, A. Coppolecchia, G. De Gasperis, M. De Leo, S. Dheilly, C. Duca, L. Dumoulin, A. Etchegoyen, A. Fasciszewski, L. P. Ferreyro, D. Fracchia, C. Franceschet, K. M. Ganga, B. García, M. E. García Redondo, M. Gaspard, D. Gayer, M. Gervasi, M. Giard, V. Gilles, Y. Giraud-Heraud, M. Gómez Berisso, M. González, M. Gradziel, M. R. Hampel, D. Harari, S. Henrot-Versillé, E. Jules, J. Kaplan, C. Kristukat, L. Lamagna, S. Loucatos, T. Louis, B. Maffei, S. Mandelli, W. Marty, A. Mattei, A. May, M. McCulloch, L. Mele, D. Melo, L. Montier, L. M. Mundo, J. A. Murphy, F. Nati, E. Olivieri, C. Oriol, A. Paiella, F. Pajot, A. Passerini, H. Pastoriza, A. Pelosi, C. Perbost, M. Perciballi, F. Pezzotta, F. Piacentini, L. Piccirillo, G. Pisano, M. Platino, G. Polenta, D. Prêle, R. Puddu, D. Rambaud, E. Rasztocky, P. Ringegni, G. E. Romero, J. M. Salum, A. Schillaci, S. Scully, S. Spinelli, G. Stankowiak, A. D. Supanitsky, P. Timbie, M. Tomasi, C. Tucker, G. Tucker, D. Viganò, N. Vittorio, F. Wicek, M. Wright, A. Zullo

Astronomy and Astrophysics Theory Group

Research output: Contribution to journal › Article › peer-review

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.

Original language	English
Article number	035
Pages (from-to)	1-27
Number of pages	27
Journal	Journal of Cosmology and Astroparticle Physics
Volume	2022
Issue number	4
DOIs	https://doi.org/10.1088/1475-7516/2022/04/035
Publication status	Published - 21 Apr 2022

Keywords

CMBR experiments
CMBR theory
cosmological parameters from CMBR
gravitational waves and CMBR polarization

Research Beacons, Institutes and Platforms

Manchester Cancer Research Centre

Access to Document

10.1088/1475-7516/2022/04/035

https://arxiv.org/pdf/2010.15119.pdf

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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. C., Incardona, F., Landau, S., Marnieros, S., Masi, S., Mennella, A., O'Sullivan, C., Piat, M., Ricciardi, G., Scóccola, C. G., ... Zullo, A. (2022). QUBIC II: Spectral polarimetry with bolometric interferometry. Journal of Cosmology and Astroparticle Physics, 2022(4), 1-27. Article 035. https://doi.org/10.1088/1475-7516/2022/04/035

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title = "QUBIC II: Spectral polarimetry with bolometric interferometry",

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. ",

keywords = "CMBR experiments, CMBR theory, cosmological parameters from CMBR, gravitational waves and CMBR polarization",

author = "L. Mousset and {Gamboa Lerena}, {M. M.} and Battistelli, {E. S.} and {De Bernardis}, P. and P. Chanial and G. D'Alessandro and G. Dashyan and {De Petris}, M. and L. Grandsire and Hamilton, {J. Ch} and F. Incardona and S. Landau and S. Marnieros and S. Masi and A. Mennella and C. O'Sullivan and M. Piat and G. Ricciardi and Sc{\'o}ccola, {C. G.} and M. Stolpovskiy and A. Tartari and Thermeau, {J. P.} and Torchinsky, {S. A.} and F. Voisin and M. Zannoni and P. Ade and Alberro, {J. G.} and A. Almela and G. Amico and Arnaldi, {L. H.} and D. Auguste and J. Aumont and S. Azzoni and S. Banfi and A. Ba{\`u} and B. B{\'e}lier and D. Bennett and L. Berg{\'e} and Bernard, {J. Ph} and M. Bersanelli and Bigot-Sazy, {M. A.} and J. Bonaparte and J. Bonis and E. Bunn and D. Burke and D. Buzi and F. Cavaliere and C. Chapron and R. Charlassier and {Cobos Cerutti}, {A. C.} and F. Columbro and A. Coppolecchia and {De Gasperis}, G. and {De Leo}, M. and S. Dheilly and C. Duca and L. Dumoulin and A. Etchegoyen and A. Fasciszewski and Ferreyro, {L. P.} and D. Fracchia and C. Franceschet and Ganga, {K. M.} and B. Garc{\'i}a and {Garc{\'i}a Redondo}, {M. E.} and M. Gaspard and D. Gayer and M. Gervasi and M. Giard and V. Gilles and Y. Giraud-Heraud and {G{\'o}mez Berisso}, M. and M. Gonz{\'a}lez and M. Gradziel and Hampel, {M. R.} and D. Harari and S. Henrot-Versill{\'e} and E. Jules and J. Kaplan and C. Kristukat and L. Lamagna and S. Loucatos and T. Louis and B. Maffei and S. Mandelli and W. Marty and A. Mattei and A. May and M. McCulloch and L. Mele and D. Melo and L. Montier and Mundo, {L. M.} and Murphy, {J. A.} and F. Nati and E. Olivieri and C. Oriol and A. Paiella and F. Pajot and A. Passerini and H. Pastoriza and A. Pelosi and C. Perbost and M. Perciballi and F. Pezzotta and F. Piacentini and L. Piccirillo and G. Pisano and M. Platino and G. Polenta and D. Pr{\^e}le and R. Puddu and D. Rambaud and E. Rasztocky and P. Ringegni and Romero, {G. E.} and Salum, {J. M.} and A. Schillaci and S. Scully and S. Spinelli and G. Stankowiak and Supanitsky, {A. D.} and P. Timbie and M. Tomasi and C. Tucker and G. Tucker and D. Vigan{\`o} and N. Vittorio and F. Wicek and M. Wright and A. Zullo",

note = "Publisher Copyright: {\textcopyright} 2022 IOP Publishing Ltd and Sissa Medialab.",

year = "2022",

month = apr,

day = "21",

doi = "10.1088/1475-7516/2022/04/035",

language = "English",

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pages = "1--27",

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Mousset, L, Gamboa Lerena, MM, Battistelli, ES, De Bernardis, P, Chanial, P, D'Alessandro, G, Dashyan, G, De Petris, M, Grandsire, L, Hamilton, JC, Incardona, F, Landau, S, Marnieros, S, Masi, S, Mennella, A, O'Sullivan, C, Piat, M, Ricciardi, G, Scóccola, CG, Stolpovskiy, M, Tartari, A, Thermeau, JP, Torchinsky, SA, Voisin, F, Zannoni, M, Ade, P, Alberro, JG, Almela, A, Amico, G, Arnaldi, LH, Auguste, D, Aumont, J, Azzoni, S, Banfi, S, Baù, A, Bélier, B, Bennett, D, Bergé, L, Bernard, JP, Bersanelli, M, Bigot-Sazy, MA, Bonaparte, J, Bonis, J, Bunn, E, Burke, D, Buzi, D, Cavaliere, F, Chapron, C, Charlassier, R, Cobos Cerutti, AC, Columbro, F, Coppolecchia, A, De Gasperis, G, De Leo, M, Dheilly, S, Duca, C, Dumoulin, L, Etchegoyen, A, Fasciszewski, A, Ferreyro, LP, Fracchia, D, Franceschet, C, Ganga, KM, García, B, García Redondo, ME, Gaspard, M, Gayer, D, Gervasi, M, Giard, M, Gilles, V, Giraud-Heraud, Y, Gómez Berisso, M, González, M, Gradziel, M, Hampel, MR, 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, LM, Murphy, JA, 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, GE, Salum, JM, Schillaci, A, Scully, S, Spinelli, S, Stankowiak, G, Supanitsky, AD, Timbie, P, Tomasi, M, Tucker, C, Tucker, G, Viganò, D, Vittorio, N, Wicek, F, Wright, M & Zullo, A 2022, 'QUBIC II: Spectral polarimetry with bolometric interferometry', Journal of Cosmology and Astroparticle Physics, vol. 2022, no. 4, 035, pp. 1-27. https://doi.org/10.1088/1475-7516/2022/04/035

TY - JOUR

T1 - QUBIC II

T2 - Spectral polarimetry with bolometric interferometry

AU - Mousset, L.

AU - Gamboa Lerena, M. M.

AU - Battistelli, E. S.

AU - De Bernardis, P.

AU - Chanial, P.

AU - D'Alessandro, G.

AU - Dashyan, G.

AU - De Petris, M.

AU - Grandsire, L.

AU - Hamilton, J. Ch

AU - Incardona, F.

AU - Landau, S.

AU - Marnieros, S.

AU - Masi, S.

AU - Mennella, A.

AU - O'Sullivan, C.

AU - Piat, M.

AU - Ricciardi, G.

AU - Scóccola, C. G.

AU - Stolpovskiy, M.

AU - Tartari, A.

AU - Thermeau, J. P.

AU - Torchinsky, S. A.

AU - Voisin, F.

AU - Zannoni, M.

AU - Ade, P.

AU - Alberro, J. G.

AU - Almela, A.

AU - Amico, G.

AU - Arnaldi, L. H.

AU - Auguste, D.

AU - Aumont, J.

AU - Azzoni, S.

AU - Banfi, S.

AU - Baù, A.

AU - Bélier, B.

AU - Bennett, D.

AU - Bergé, L.

AU - Bernard, J. Ph

AU - Bersanelli, M.

AU - Bigot-Sazy, M. A.

AU - Bonaparte, J.

AU - Bonis, J.

AU - Bunn, E.

AU - Burke, D.

AU - Buzi, D.

AU - Cavaliere, F.

AU - Chapron, C.

AU - Charlassier, R.

AU - Cobos Cerutti, A. C.

AU - Columbro, F.

AU - Coppolecchia, A.

AU - De Gasperis, G.

AU - De Leo, M.

AU - Dheilly, S.

AU - Duca, C.

AU - Dumoulin, L.

AU - Etchegoyen, A.

AU - Fasciszewski, A.

AU - Ferreyro, L. P.

AU - Fracchia, D.

AU - Franceschet, C.

AU - Ganga, K. M.

AU - García, B.

AU - García Redondo, M. E.

AU - Gaspard, M.

AU - Gayer, D.

AU - Gervasi, M.

AU - Giard, M.

AU - Gilles, V.

AU - Giraud-Heraud, Y.

AU - Gómez Berisso, M.

AU - González, M.

AU - Gradziel, M.

AU - Hampel, M. R.

AU - Harari, D.

AU - Henrot-Versillé, S.

AU - Jules, E.

AU - Kaplan, J.

AU - Kristukat, C.

AU - Lamagna, L.

AU - Loucatos, S.

AU - Louis, T.

AU - Maffei, B.

AU - Mandelli, S.

AU - Marty, W.

AU - Mattei, A.

AU - May, A.

AU - McCulloch, M.

AU - Mele, L.

AU - Melo, D.

AU - Montier, L.

AU - Mundo, L. M.

AU - Murphy, J. A.

AU - Nati, F.

AU - Olivieri, E.

AU - Oriol, C.

AU - Paiella, A.

AU - Pajot, F.

AU - Passerini, A.

AU - Pastoriza, H.

AU - Pelosi, A.

AU - Perbost, C.

AU - Perciballi, M.

AU - Pezzotta, F.

AU - Piacentini, F.

AU - Piccirillo, L.

AU - Pisano, G.

AU - Platino, M.

AU - Polenta, G.

AU - Prêle, D.

AU - Puddu, R.

AU - Rambaud, D.

AU - Rasztocky, E.

AU - Ringegni, P.

AU - Romero, G. E.

AU - Salum, J. M.

AU - Schillaci, A.

AU - Scully, S.

AU - Spinelli, S.

AU - Stankowiak, G.

AU - Supanitsky, A. D.

AU - Timbie, P.

AU - Tomasi, M.

AU - Tucker, C.

AU - Tucker, G.

AU - Viganò, D.

AU - Vittorio, N.

AU - Wicek, F.

AU - Wright, M.

AU - Zullo, A.

PY - 2022/4/21

Y1 - 2022/4/21

N2 - 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.

AB - 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.

KW - CMBR experiments

KW - CMBR theory

KW - cosmological parameters from CMBR

KW - gravitational waves and CMBR polarization

UR - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=pure_starter&SrcAuth=WosAPI&KeyUT=WOS:000807377200005&DestLinkType=FullRecord&DestApp=WOS

UR - https://www.mendeley.com/catalogue/18011b9f-1ecd-3891-b04e-b0fb79cabfaf/

U2 - 10.1088/1475-7516/2022/04/035

DO - 10.1088/1475-7516/2022/04/035

M3 - Article

AN - SCOPUS:85129905523

SN - 1475-7516

VL - 2022

SP - 1

EP - 27

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 4

M1 - 035

ER -

QUBIC II: Spectral polarimetry with bolometric interferometry

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Keywords

Research Beacons, Institutes and Platforms

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