Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps
- de Zotti, G.
- González-Nuevo, J.
- Lopez-Caniego, M.
- Negrello, M.
- Greenslade, J.
- Hernández-Monteagudo, C.
- Delabrouille, J.
- Cai, Z.-Y.
- Bonato, M.
- Achúcarro, A.
- Ade, P.
- Allison, R.
- Ashdown, M.
- Ballardini, M.
- Banday, A.J.
- Banerji, R.
- Bartlett, J.G.
- Bartolo, N.
- Basak, S.
- Bersanelli, M.
- Biesiada, M.
- Bilicki, M.
- Bonaldi, A.
- Borrill, J.
- Bouchet, F.
- Boulanger, F.
- Brinckmann, T.
- Bucher, M.
- Burigana, C.
- Buzzelli, A.
- Calvo, M.
- Carvalho, C.S.
- Castellano, M.G.
- Challinor, A.
- Chluba, J.
- Clements, D.L.
- Clesse, S.
- Colafrancesco, S.
- Colantoni, I.
- Coppolecchia, A.
- Crook, M.
- d'Alessandro, G.
- de Bernardis, P.
- de Gasperis, G.
- Diego, J.M.
- Di Valentino, E.
- Errard, J.
- Feeney, S.M.
- Fernández-Cobos, R.
- Ferraro, S.
- Finelli, F.
- Forastieri, F.
- Galli, S.
- Génova-Santos, R.T.
- Gerbino, M.
- Grandis, S.
- Hagstotz, S.
- Hanany, S.
- Handley, W.
- Hervias-Caimapo, C.
- Hills, M.
- Hivon, E.
- Kiiveri, K.
- Kisner, T.
- Kitching, T.
- Kunz, M.
- Kurki-Suonio, H.
- Lagache, G.
- Lamagna, L.
- Lasenby, A.
- Lattanzi, M.
- Le Brun, A.
- Lesgourgues, J.
- Lewis, A.
- Liguori, M.
- Lindholm, V.
- Luzzi, G.
- Maffei, B.
- Mandolesi, N.
- Martinez-Gonzalez, E.
- Martins, C.J.A.P.
- Masi, S.
- Massardi, M.
- Mccarthy, D.
- Melchiorri, A.
- Melin, J.-B.
- Molinari, D.
- Monfardini, A.
- Natoli, P.
- Notari, A.
- Paiella, A.
- Paoletti, D.
- Partridge, R.B.
- Patanchon, G.
- Piat, M.
- Pisano, G.
- Polastri, L.
- Polenta, G.
- Pollo, A.
- Poulin, V.
- Quartin, M.
- Remazeilles, M.
- Roman, M.
- Rossi, G.
- Roukema, B.F.
- Rubino-Martin, J.-A.
- Salvati, L.
- Scott, D.
- Serjeant, S.
- Tartari, A.
- Toffolatti, L.
- Tomasi, M.
- Trappe, N.
- Triqueneaux, S.
- Trombetti, T.
- Tucci, M.
- Tucker, C.
- Väliviita, J.
- van de Weygaert, R.
- van Tent, B.
- Vennin, Vincent
- Vielva, P.
- Vittorio, N.
- Young, K.
DOIAbstract
International audienceWe discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on the definition of the future space project, CORE, that has been submitted in response to ESA's call for a Medium-size mission opportunity as the successor of the Planck satellite. Even though the effective telescope size will be somewhat smaller than that of Planck, CORE will have a considerably better angular resolution at its highest frequencies, since, in contrast with Planck, it will be diffraction limited at all frequencies. The improved resolution implies a considerable decrease of the source confusion, i.e. substantially fainter detect...
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