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Exploring Cosmic Origins with CORE: Survey requirements and mission design

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arxiv 1706.04516 v1 pith:PJ2Y4CXD submitted 2017-06-14 astro-ph.IM astro-ph.CO

Exploring Cosmic Origins with CORE: Survey requirements and mission design

J. Delabrouille , P. de Bernardis , F. R. Bouchet , A. Ach\'ucarro , P. A. R. Ade , R. Allison , F. Arroja , E. Artal
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M. Ashdown C. Baccigalupi M. Ballardini A. J. Banday R. Banerji D. Barbosa J. Bartlett N. Bartolo S. Basak J. J. A. Baselmans K. Basu E. S. Battistelli R. Battye D. Baumann A. Beno\^it M. Bersanelli A. Bideaud M. Biesiada M. Bilicki A. Bonaldi M. Bonato J. Borrill F. Boulanger T. Brinckmann M. L. Brown M. Bucher C. Burigana A. Buzzelli G. Cabass Z.-Y. Cai M. Calvo A. Caputo C.-S. Carvalho F. J. Casas G. Castellano A. Catalano A. Challinor I. Charles J. Chluba D. L. Clements S. Clesse S. Colafrancesco I. Colantoni D. Contreras A. Coppolecchia M. Crook G. D'Alessandro G. D'Amico A. da Silva M. de Avillez G. de Gasperis M. De Petris G. de Zotti L. Danese F.-X. D\'esert V. Desjacques E. Di Valentino C. Dickinson J. M. Diego S. Doyle R. Durrer C. Dvorkin H.-K. Eriksen J. Errard S. Feeney R. Fern\'andez-Cobos F. Finelli F. Forastieri C. Franceschet U. Fuskeland S. Galli R. T. G\'enova-Santos M. Gerbino E. Giusarma A. Gomez J. Gonz\'alez-Nuevo S. Grandis J. Greenslade J. Goupy S. Hagstotz S. Hanany W. Handley S. Henrot-Versill\'e C. Hern\'andez-Monteagudo C. Hervias-Caimapo M. Hills M. Hindmarsh E. Hivon D. T. Hoang D. C. Hooper B. Hu E. Keih\"anen R. Keskitalo K. Kiiveri T. Kisner T. Kitching M. Kunz H. Kurki-Suonio G. Lagache L. Lamagna A. Lapi A. Lasenby M. Lattanzi A. M. C. Le Brun J. Lesgourgues M. Liguori V. Lindholm J. Lizarraga G. Luzzi J. F. Mac\`ias-P\'erez B. Maffei N. Mandolesi S. Martin E. Martinez-Gonzalez C.J.A.P. Martins S. Masi M. Massardi S. Matarrese P. Mazzotta D. McCarthy A. Melchiorri J.-B. Melin A. Mennella J. Mohr D. Molinari A. Monfardini L. Montier P. Natoli M. Negrello A. Notari F. Noviello F. Oppizzi C. O'Sullivan L. Pagano A. Paiella E. Pajer D. Paoletti S. Paradiso R. B. Partridge G. Patanchon S. P. Patil O. Perdereau F. Piacentini M. Piat G. Pisano L. Polastri G. Polenta A. Pollo N. Ponthieu V. Poulin D. Pr\^ele M. Quartin A. Ravenni M. Remazeilles A. Renzi C. Ringeval D. Roest M. Roman B. F. Roukema J.-A. Rubino-Martin L. Salvati D. Scott S. Serjeant G. Signorelli A. A. Starobinsky R. Sunyaev C. Y. Tan A. Tartari G. Tasinato L. Toffolatti M. Tomasi J. Torrado D. Tramonte N. Trappe S. Triqueneaux M. Tristram T. Trombetti M. Tucci C. Tucker J. Urrestilla J. V\"aliviita R. Van de Weygaert B. Van Tent V. Vennin L. Verde G. Vermeulen P. Vielva N. Vittorio F. Voisin C. Wallis B. Wandelt I. Wehus J. Weller K. Young M. Zannoni (for the CORE collaboration)
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classification astro-ph.IM astro-ph.CO
keywords missionpolarisationcoredesignfutureobservationsanswercosmic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE is designed as a near-ultimate CMB polarisation mission which, for optimal complementarity with ground-based observations, will perform the observations that are known to be essential to CMB polarisation scienceand cannot be obtained by any other means than a dedicated space mission.

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