Exploring cosmic origins with CORE: The instrument

P. De Bernardis; P. A.R. Ade; J. J.A. Baselmans; E. S. Battistelli; A. Benoit; M. Bersanelli; A. Bideaud; M. Calvo; F. J. Casas; M. G. Castellano; A. Catalano; I. Charles; I. Colantoni; F. Columbro; A. Coppolecchia; M. Crook; G. D'Alessandro; M. De Petris; J. Delabrouille; S. Doyle; C. Franceschet; A. Gomez; J. Goupy; S. Hanany; M. Hills; L. Lamagna; J. Macias-Perez; B. Maffei; S. Martin; E. Martinez-Gonzalez; S. Masi; D. McCarthy; A. Mennella; A. Monfardini; F. Noviello; A. Paiella; F. Piacentini; M. Piat; G. Pisano; G. Signorelli; C. Y. Tan; A. Tartari; N. Trappe; S. Triqueneaux; C. Tucker; G. Vermeulen; K. Young; M. Zannoni; A. Achúcarro; R. Allison; E. Artall; M. Ashdown; M. Ballardini; A. J. Banday; R. Banerji; J. Bartlett; N. Bartolo; S. Basak; A. Bonaldi; M. Bonato; J. Borrill; F. Bouchet; F. Boulanger; T. Brinckmann; M. Bucher; C. Burigana; A. Buzzelli; Z. Y. Cai; C. S. Carvalho; A. Challinor; J. Chluba; S. Clesse; G. De Gasperis; G. De Zotti; E. Di Valentino; J. M. Diego; J. Errard; S. Feeney; R. Fernandez-Cobos; F. Finelli; F. Forastieri; S. Galli; R. Génova-Santos; M. Gerbino; J. González-Nuevo; S. Hagstotz; J. Greenslade; W. Handley; C. Hernández-Monteagudo; C. Hervias-Caimapo; E. Hivon; K. Kiiveri; T. Kisner; T. Kitching; M. Kunz; H. Kurki-Suonio; A. Lasenby; M. Lattanzi; J. Lesgourgues; A. Lewis; M. Liguori; V. Lindholm; G. Luzzi; C. J.A.P. Martins; S. Matarrese; A. Melchiorri; J. B. Melin; D. Molinari; P. Natoli; M. Negrello; A. Notari; D. Paoletti; G. Patanchon; L. Polastri; G. Polenta; A. Pollo; V. Poulin; M. Quartin; M. Remazeilles; M. Roman; J. A. Rubiño-Martín; L. Salvati; M. Tomasi; D. Tramonte; T. Trombetti; J. Väliviita; R. Van De Weyjgaert; B. Van Tent; V. Vennin; P. Vielva; N. Vittorio

doi:10.1088/1475-7516/2018/04/015

Exploring cosmic origins with CORE: The instrument

P. De Bernardis
, P. A.R. Ade
, J. J.A. Baselmans
, E. S. Battistelli
, A. Benoit
, M. Bersanelli
, A. Bideaud
, M. Calvo
, F. J. Casas
, M. G. Castellano
, A. Catalano
, I. Charles
, I. Colantoni
, F. Columbro
, A. Coppolecchia
, M. Crook
, G. D'Alessandro
, M. De Petris
, J. Delabrouille
, S. Doyle

C. Franceschet, A. Gomez, J. Goupy, S. Hanany, M. Hills, L. Lamagna, J. Macias-Perez, B. Maffei, S. Martin, E. Martinez-Gonzalez, S. Masi, D. McCarthy, A. Mennella, A. Monfardini, F. Noviello, A. Paiella, F. Piacentini, M. Piat, G. Pisano, G. Signorelli, C. Y. Tan, A. Tartari, N. Trappe, S. Triqueneaux, C. Tucker, G. Vermeulen, K. Young, M. Zannoni, A. Achúcarro, R. Allison, E. Artall, M. Ashdown, M. Ballardini, A. J. Banday, R. Banerji, J. Bartlett, N. Bartolo, S. Basak, A. Bonaldi, M. Bonato, J. Borrill, F. Bouchet, F. Boulanger, T. Brinckmann, M. Bucher, C. Burigana, A. Buzzelli, Z. Y. Cai, C. S. Carvalho, A. Challinor, J. Chluba, S. Clesse, G. De Gasperis, G. De Zotti, E. Di Valentino, J. M. Diego, J. Errard, S. Feeney, R. Fernandez-Cobos, F. Finelli, F. Forastieri, S. Galli, R. Génova-Santos, M. Gerbino, J. González-Nuevo, S. Hagstotz, J. Greenslade, W. Handley, C. Hernández-Monteagudo, C. Hervias-Caimapo, E. Hivon, K. Kiiveri, T. Kisner, T. Kitching, M. Kunz, H. Kurki-Suonio, A. Lasenby, M. Lattanzi, J. Lesgourgues, A. Lewis, M. Liguori, V. Lindholm, G. Luzzi, C. J.A.P. Martins, S. Matarrese, A. Melchiorri, J. B. Melin, D. Molinari, P. Natoli, M. Negrello, A. Notari, D. Paoletti, G. Patanchon, L. Polastri, G. Polenta, A. Pollo, V. Poulin, M. Quartin, M. Remazeilles, M. Roman, J. A. Rubiño-Martín, L. Salvati, M. Tomasi, D. Tramonte, T. Trombetti, J. Väliviita, R. Van De Weyjgaert, B. Van Tent, V. Vennin, P. Vielva, N. Vittorio

Dipartimento di Fisica
Sezione di Roma
Cardiff University
SRON - Netherlands Institute for Space Research
LTHE (UMR 5564 CNRS/IRD/Université de Grenoble)
University of Milano
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Instituto de Fisica de Cantabria (CSIC-UC)
CNR - IFN
CCLRC Rutherford Appleton Laboratory
Astroparticule and Cosmol APC
ESAC campus
University of Minnesota
Institut d'Astrophysique Spatiale
Maynooth University
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
University of Milano-Bicocca
Universiteit Leiden
University of the Basque Country
Institute of Astronomy
CSIC-Univ. Cantabria
University of Cambridge
University of Cambridge
University of Bologna
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
INFN Sezione di Bologna
IRAP/CNRS
University of Padova
INFN
INAF Osservatorio Astronomico di Padova
School of Biotechnology
International School of Advanced Studies
University of Manchester
Tufts University
Ernest Orlando Lawrence Berkeley National Laboratory
University of California, Space Sciences Laboratory
CNRS
RWTH Aachen University
University of Ferrara
University of Rome “Tor Vergata”
University of Science and Technology of China
Universidade de Lisboa
Sorbonne Université
Universités Paris VI and VII
Imperial College London
Center for Computational Astrophysics
Sezione INFN di Ferrara
Instituto de Astrofisica de Canarias
Research Unit; CIBERNED and Universidad de La Laguna
Stockholm University
University of Oviedo
Universität München
Technische Universität München
Centro de Estudios de Física del Cosmos de Aragón (CEFCA)
University of Helsinki
UCL Mullard Space Science Laboratory
University of Geneva
University of Sussex
Ipatimup Diagnósticos
Institut Pierre Simon Laplace, CNRS and CEA
University of Barcelona
Science and Research Directorate
Osservatorio Astronomico di Roma
National Centre for Nuclear Research (NCBJ)
Jagiellonian University
Université Savoie Mont Blanc
Instituto de Biofisica da UFRJ
University of Groningen
Université Paris-Sud
University of Portsmouth

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget requirements of a medium-size space mission within the Cosmic Vision Programme of the European Space Agency. The instrument has no moving parts, and uses arrays of diffraction-limited Kinetic Inductance Detectors to cover the frequency range from 60 GHz to 600 GHz in 19 wide bands, in the focal plane of a 1.2 m aperture telescope cooled at 40 K, allowing for an accurate extraction of the CMB signal from polarized foreground emission. The projected CMB polarization survey sensitivity of this instrument, after foregrounds removal, is 1.7 μKċarcmin. The design is robust enough to allow, if needed, a downscoped version of the instrument covering the 100 GHz to 600 GHz range with a 0.8 m aperture telescope cooled at 85 K, with a projected CMB polarization survey sensitivity of 3.2 μKċarcmin.

langue originale	Anglais
Numéro d'article	015
journal	Journal of Cosmology and Astroparticle Physics
Volume	2018
Numéro de publication	4
Les DOIs	https://doi.org/10.1088/1475-7516/2018/04/015
état	Publié - 5 avr. 2018
Modification externe	Oui

Accès au document

10.1088/1475-7516/2018/04/015

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De Bernardis, P., Ade, P. A. R., Baselmans, J. J. A., Battistelli, E. S., Benoit, A., Bersanelli, M., Bideaud, A., Calvo, M., Casas, F. J., Castellano, M. G., Catalano, A., Charles, I., Colantoni, I., Columbro, F., Coppolecchia, A., Crook, M., D'Alessandro, G., Petris, M. D., Delabrouille, J., ... Vittorio, N. (2018). Exploring cosmic origins with CORE: The instrument. Journal of Cosmology and Astroparticle Physics, 2018(4), Article 015. https://doi.org/10.1088/1475-7516/2018/04/015

@article{a0eab6fb6ca2405081fe335155c11520,

title = "Exploring cosmic origins with CORE: The instrument",

abstract = "We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget requirements of a medium-size space mission within the Cosmic Vision Programme of the European Space Agency. The instrument has no moving parts, and uses arrays of diffraction-limited Kinetic Inductance Detectors to cover the frequency range from 60 GHz to 600 GHz in 19 wide bands, in the focal plane of a 1.2 m aperture telescope cooled at 40 K, allowing for an accurate extraction of the CMB signal from polarized foreground emission. The projected CMB polarization survey sensitivity of this instrument, after foregrounds removal, is 1.7 μKċarcmin. The design is robust enough to allow, if needed, a downscoped version of the instrument covering the 100 GHz to 600 GHz range with a 0.8 m aperture telescope cooled at 85 K, with a projected CMB polarization survey sensitivity of 3.2 μKċarcmin.",

keywords = "CMBR detectors, CMBR experiments, CMBR polarization, ination",

author = "\{De Bernardis\}, P. and Ade, \{P. A.R.\} and Baselmans, \{J. J.A.\} and Battistelli, \{E. S.\} and A. Benoit and M. Bersanelli and A. Bideaud and M. Calvo and Casas, \{F. J.\} and Castellano, \{M. G.\} and A. Catalano and I. Charles and I. Colantoni and F. Columbro and A. Coppolecchia and M. Crook and G. D'Alessandro and Petris, \{M. De\} and J. Delabrouille and S. Doyle and C. Franceschet and A. Gomez and J. Goupy and S. Hanany and M. Hills and L. Lamagna and J. Macias-Perez and B. Maffei and S. Martin and E. Martinez-Gonzalez and S. Masi and D. McCarthy and A. Mennella and A. Monfardini and F. Noviello and A. Paiella and F. Piacentini and M. Piat and G. Pisano and G. Signorelli and Tan, \{C. Y.\} and A. Tartari and N. Trappe and S. Triqueneaux and C. Tucker and G. Vermeulen and K. Young and M. Zannoni and A. Ach{\'u}carro and R. Allison and E. Artall and M. Ashdown and M. Ballardini and Banday, \{A. J.\} and R. Banerji and J. Bartlett and N. Bartolo and S. Basak and A. Bonaldi and M. Bonato and J. Borrill and F. Bouchet and F. Boulanger and T. Brinckmann and M. Bucher and C. Burigana and A. Buzzelli and Cai, \{Z. Y.\} and Carvalho, \{C. S.\} and A. Challinor and J. Chluba and S. Clesse and Gasperis, \{G. De\} and Zotti, \{G. De\} and Valentino, \{E. Di\} and Diego, \{J. M.\} and J. Errard and S. Feeney and R. Fernandez-Cobos and F. Finelli and F. Forastieri and S. Galli and R. G{\'e}nova-Santos and M. Gerbino and J. Gonz{\'a}lez-Nuevo and S. Hagstotz and J. Greenslade and W. Handley and C. Hern{\'a}ndez-Monteagudo and C. Hervias-Caimapo and E. Hivon and K. Kiiveri and T. Kisner and T. Kitching and M. Kunz and H. Kurki-Suonio and A. Lasenby and M. Lattanzi and J. Lesgourgues and A. Lewis and M. Liguori and V. Lindholm and G. Luzzi and Martins, \{C. J.A.P.\} and S. Matarrese and A. Melchiorri and Melin, \{J. B.\} and D. Molinari and P. Natoli and M. Negrello and A. Notari and D. Paoletti and G. Patanchon and L. Polastri and G. Polenta and A. Pollo and V. Poulin and M. Quartin and M. Remazeilles and M. Roman and Rubi{\~n}o-Mart{\'i}n, \{J. A.\} and L. Salvati and M. Tomasi and D. Tramonte and T. Trombetti and J. V{\"a}liviita and \{De Weyjgaert\}, \{R. Van\} and Tent, \{B. Van\} and V. Vennin and P. Vielva and N. Vittorio",

note = "Publisher Copyright: {\textcopyright} 2018 IOP Publishing Ltd and Sissa Medialab.",

year = "2018",

month = apr,

day = "5",

doi = "10.1088/1475-7516/2018/04/015",

language = "English",

volume = "2018",

journal = "Journal of Cosmology and Astroparticle Physics",

issn = "1475-7516",

number = "4",

}

De Bernardis, P, Ade, PAR, Baselmans, JJA, Battistelli, ES, Benoit, A, Bersanelli, M, Bideaud, A, Calvo, M, Casas, FJ, Castellano, MG, Catalano, A, Charles, I, Colantoni, I, Columbro, F, Coppolecchia, A, Crook, M, D'Alessandro, G, Petris, MD, Delabrouille, J, Doyle, S, Franceschet, C, Gomez, A, Goupy, J, Hanany, S, Hills, M, Lamagna, L, Macias-Perez, J, Maffei, B, Martin, S, Martinez-Gonzalez, E, Masi, S, McCarthy, D, Mennella, A, Monfardini, A, Noviello, F, Paiella, A, Piacentini, F, Piat, M, Pisano, G, Signorelli, G, Tan, CY, Tartari, A, Trappe, N, Triqueneaux, S, Tucker, C, Vermeulen, G, Young, K, Zannoni, M, Achúcarro, A, Allison, R, Artall, E, Ashdown, M, Ballardini, M, Banday, AJ, Banerji, R, Bartlett, J, Bartolo, N, Basak, S, Bonaldi, A, Bonato, M, Borrill, J, Bouchet, F, Boulanger, F, Brinckmann, T, Bucher, M, Burigana, C, Buzzelli, A, Cai, ZY, Carvalho, CS, Challinor, A, Chluba, J, Clesse, S, Gasperis, GD, Zotti, GD, Valentino, ED, Diego, JM, Errard, J, Feeney, S, Fernandez-Cobos, R, Finelli, F, Forastieri, F, Galli, S, Génova-Santos, R, Gerbino, M, González-Nuevo, J, Hagstotz, S, Greenslade, J, Handley, W, Hernández-Monteagudo, C, Hervias-Caimapo, C, Hivon, E, Kiiveri, K, Kisner, T, Kitching, T, Kunz, M, Kurki-Suonio, H, Lasenby, A, Lattanzi, M, Lesgourgues, J, Lewis, A, Liguori, M, Lindholm, V, Luzzi, G, Martins, CJAP, Matarrese, S, Melchiorri, A, Melin, JB, Molinari, D, Natoli, P, Negrello, M, Notari, A, Paoletti, D, Patanchon, G, Polastri, L, Polenta, G, Pollo, A, Poulin, V, Quartin, M, Remazeilles, M, Roman, M, Rubiño-Martín, JA, Salvati, L, Tomasi, M, Tramonte, D, Trombetti, T, Väliviita, J, De Weyjgaert, RV, Tent, BV, Vennin, V, Vielva, P & Vittorio, N 2018, 'Exploring cosmic origins with CORE: The instrument', Journal of Cosmology and Astroparticle Physics, VOL. 2018, Numéro 4, 015. https://doi.org/10.1088/1475-7516/2018/04/015

TY - JOUR

T1 - Exploring cosmic origins with CORE

T2 - The instrument

AU - De Bernardis, P.

AU - Ade, P. A.R.

AU - Baselmans, J. J.A.

AU - Battistelli, E. S.

AU - Benoit, A.

AU - Bersanelli, M.

AU - Bideaud, A.

AU - Calvo, M.

AU - Casas, F. J.

AU - Castellano, M. G.

AU - Catalano, A.

AU - Charles, I.

AU - Colantoni, I.

AU - Columbro, F.

AU - Coppolecchia, A.

AU - Crook, M.

AU - D'Alessandro, G.

AU - Petris, M. De

AU - Delabrouille, J.

AU - Doyle, S.

AU - Franceschet, C.

AU - Gomez, A.

AU - Goupy, J.

AU - Hanany, S.

AU - Hills, M.

AU - Lamagna, L.

AU - Macias-Perez, J.

AU - Maffei, B.

AU - Martin, S.

AU - Martinez-Gonzalez, E.

AU - Masi, S.

AU - McCarthy, D.

AU - Mennella, A.

AU - Monfardini, A.

AU - Noviello, F.

AU - Paiella, A.

AU - Piacentini, F.

AU - Piat, M.

AU - Pisano, G.

AU - Signorelli, G.

AU - Tan, C. Y.

AU - Tartari, A.

AU - Trappe, N.

AU - Triqueneaux, S.

AU - Tucker, C.

AU - Vermeulen, G.

AU - Young, K.

AU - Zannoni, M.

AU - Achúcarro, A.

AU - Allison, R.

AU - Artall, E.

AU - Ashdown, M.

AU - Ballardini, M.

AU - Banday, A. J.

AU - Banerji, R.

AU - Bartlett, J.

AU - Bartolo, N.

AU - Basak, S.

AU - Bonaldi, A.

AU - Bonato, M.

AU - Borrill, J.

AU - Bouchet, F.

AU - Boulanger, F.

AU - Brinckmann, T.

AU - Bucher, M.

AU - Burigana, C.

AU - Buzzelli, A.

AU - Cai, Z. Y.

AU - Carvalho, C. S.

AU - Challinor, A.

AU - Chluba, J.

AU - Clesse, S.

AU - Gasperis, G. De

AU - Zotti, G. De

AU - Valentino, E. Di

AU - Diego, J. M.

AU - Errard, J.

AU - Feeney, S.

AU - Fernandez-Cobos, R.

AU - Finelli, F.

AU - Forastieri, F.

AU - Galli, S.

AU - Génova-Santos, R.

AU - Gerbino, M.

AU - González-Nuevo, J.

AU - Hagstotz, S.

AU - Greenslade, J.

AU - Handley, W.

AU - Hernández-Monteagudo, C.

AU - Hervias-Caimapo, C.

AU - Hivon, E.

AU - Kiiveri, K.

AU - Kisner, T.

AU - Kitching, T.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lasenby, A.

AU - Lattanzi, M.

AU - Lesgourgues, J.

AU - Lewis, A.

AU - Liguori, M.

AU - Lindholm, V.

AU - Luzzi, G.

AU - Martins, C. J.A.P.

AU - Matarrese, S.

AU - Melchiorri, A.

AU - Melin, J. B.

AU - Molinari, D.

AU - Natoli, P.

AU - Negrello, M.

AU - Notari, A.

AU - Paoletti, D.

AU - Patanchon, G.

AU - Polastri, L.

AU - Polenta, G.

AU - Pollo, A.

AU - Poulin, V.

AU - Quartin, M.

AU - Remazeilles, M.

AU - Roman, M.

AU - Rubiño-Martín, J. A.

AU - Salvati, L.

AU - Tomasi, M.

AU - Tramonte, D.

AU - Trombetti, T.

AU - Väliviita, J.

AU - De Weyjgaert, R. Van

AU - Tent, B. Van

AU - Vennin, V.

AU - Vielva, P.

AU - Vittorio, N.

PY - 2018/4/5

Y1 - 2018/4/5

N2 - We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget requirements of a medium-size space mission within the Cosmic Vision Programme of the European Space Agency. The instrument has no moving parts, and uses arrays of diffraction-limited Kinetic Inductance Detectors to cover the frequency range from 60 GHz to 600 GHz in 19 wide bands, in the focal plane of a 1.2 m aperture telescope cooled at 40 K, allowing for an accurate extraction of the CMB signal from polarized foreground emission. The projected CMB polarization survey sensitivity of this instrument, after foregrounds removal, is 1.7 μKċarcmin. The design is robust enough to allow, if needed, a downscoped version of the instrument covering the 100 GHz to 600 GHz range with a 0.8 m aperture telescope cooled at 85 K, with a projected CMB polarization survey sensitivity of 3.2 μKċarcmin.

AB - We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget requirements of a medium-size space mission within the Cosmic Vision Programme of the European Space Agency. The instrument has no moving parts, and uses arrays of diffraction-limited Kinetic Inductance Detectors to cover the frequency range from 60 GHz to 600 GHz in 19 wide bands, in the focal plane of a 1.2 m aperture telescope cooled at 40 K, allowing for an accurate extraction of the CMB signal from polarized foreground emission. The projected CMB polarization survey sensitivity of this instrument, after foregrounds removal, is 1.7 μKċarcmin. The design is robust enough to allow, if needed, a downscoped version of the instrument covering the 100 GHz to 600 GHz range with a 0.8 m aperture telescope cooled at 85 K, with a projected CMB polarization survey sensitivity of 3.2 μKċarcmin.

KW - CMBR detectors

KW - CMBR experiments

KW - CMBR polarization

KW - ination

UR - https://www.scopus.com/pages/publications/85046844703

U2 - 10.1088/1475-7516/2018/04/015

DO - 10.1088/1475-7516/2018/04/015

M3 - Article

AN - SCOPUS:85046844703

SN - 1475-7516

VL - 2018

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 4

M1 - 015

ER -

Exploring cosmic origins with CORE: The instrument

Résumé

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