Exploring cosmic origins with CORE: The instrument
- 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. De
- 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, C. Y.
- 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, A. J.
- 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, Z. Y.
- Carvalho, C. S.
- Challinor, A.
- Chluba, J.
- Clesse, S.
- Gasperis, G. De
- Zotti, G. De
- Valentino, E. Di
- Diego, J. M.
- 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, C. J. A. P.
- Matarrese, S.
- Melchiorri, A.
- Melin, J. B.
- 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, J. A.
- Salvati, L.
- Tomasi, M.
- Tramonte, D.
- Trombetti, T.
- Väliviita, J.
- De Weyjgaert, R. Van
- Tent, B. Van
- Vennin, V.
- Vielva, P.
- Vittorio, N.
DOIAbstract
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 foreg...
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