{"paper":{"title":"Exploring Cosmic Origins with CORE: The Instrument","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A. Ach\\'ucarro, A. Benoit, A. Bideaud, A. Bonaldi, A. Buzzelli, A. Catalano, A. Challinor, A. Coppolecchia, A. Gomez, A.J. Banday, A. Lasenby, A. Lewis, A. Melchiorri, A. Mennella, A. Monfardini, A. Notari, A. Paiella, A. Pollo, A. Tartari, B. Maffei, B. Van Tent, C. Burigana, C. Franceschet, C. Hern\\'andez-Monteagudo, C. Hervias-Caimapo, C.J.A.P. Martins, C.S. Carvalho, C. Tucker, C.Y. Tan, D. McCarthy, D. Molinari, D. Paoletti, D. Tramonte, E. Di Valentino, E. Hivon, E. Martinez-Gonzalez, E.S. Battistelli, F. Bouchet, F. Boulanger, F. Columbro, F. Finelli, F. Forastieri, F.J. Casas, F. Noviello, F. Piacentini, G. Castellano, G. D'Alessandro, G. De Gasperis, G. de Zotti, G. Luzzi, G. Patanchon, G. Pisano, G. Polenta, G. Signorelli, G. Vermeulen, H. Kurki-Suonio, I. Charles, I. Colantoni, J.A. Rubi\\~no-Mart\\'in, J. Bartlett, J.B. Melin, J. Borrill, J. Chluba, J. Delabrouille, J. Errard, J. Gonz\\'alez-Nuevo, J. Goupy, J. Greenslade, J.J.A. Baselmans, J. Lesgourgues, J. Macias-Perez, J.M. Diego, J. V\\\"aliviita, K. Kiiveri, K. Young, L. Lamagna, L. Polastri, L. Salvati, M. Ashdown, M. Ballardini, M. Bersanelli, M. Bonato, M. Bucher, M. Calvo, M. Crook, M. De Petris, M. Gerbino, M. Hills, M. Kunz, M. Lattanzi, M. Liguori, M. Negrello, M. Piat, M. Quartin, M. Remazeilles, M. Roman, M. Tomasi, M. Zannoni, N. Bartolo, N. Trappe, N. Vittorio (for the CORE collaboration), P.A.R. Ade, P. De Bernardis, P. Natoli, P. Vielva, R. Allison, R. Banerji, R. Fernandez-Cobos, R. G\\'enova-Santos, R. Van de Weijgaert, S. Basak, S. Clesse, S. Doyle, S. Feeney, S. Galli, S. Hagstotz, S. Hanany, S. Martin, S. Masi, S. Triqueneaux, T. Brinckmann, T. Kisner, T. Kitching, T. Trombetti, V. Lindholm, V. Poulin, V. Vennin, W. Handley, Z.Y. Cai","submitted_at":"2017-05-05T11:10:04Z","abstract_excerpt":"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 accur"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.02170","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1705.02170/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}