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| Akrami, Y.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Ballardini, M.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Basak, S.; Benabed, K.; Bernard, J-p; Bersanelli, M.; Bielewicz, P.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Burigana, C.; Calabrese, E.; Carvalho, P.; Chiang, H. C.; Crill, B. P.; Cuttaia, F.; De Rosa, A.; De Zotti, G.; Delabrouille, J.; Delouis, Jean Marc; Di Valentino, E.; Diego, J. M.; Dupac, X.; Dusini, S.; Efstathiou, G.; Elsner, F.; Ensslin, T. A.; Eriksen, H. K.; Fernandez-cobos, R.; Finelli, F.; Fraisse, A. A.; Franceschi, E.; Frolov, A.; Galeotta, S.; Ganga, K.; Gerbino, M.; Gonzalez-nuevo, J.; Gorski, K. M.; Gratton, S.; Gruppuso, A.; Gudmundsson, J. E.; Handley, W.; Hansen, F. K.; Herranz, D.; Hivon, E.; Hobson, M.; Huang, Z.; Jones, W. C.; Keihanen, E.; Keskitalo, R.; Kim, J.; Kisner, T. S.; Krachmalnicoff, N.; Kunz, M.; Kurki-suonio, H.; Lamarre, J-m; Lasenby, A.; Lattanzi, M.; Lawrence, C. R.; Le Jeune, M; Levrier, F.; Lilje, P. B.; Lindholm, V; Lopez-caniego, M.; Ma, Y-z; Macias-perez, J. F.; Maggio, G.; Mandolesi, N.; Marcos-caballero, A.; Maris, M.; Martin, Pg; Martinez-gonzalez, E.; Matarrese, S.; Mauri, N.; Mcewen, J. D.; Migliaccio, M.; Molinari, D.; Moneti, A.; Montier, L.; Morgante, G.; Natoli, P.; Paoletti, D.; Partridge, B.; Perrotta, F.; Pettorino, V; Piacentini, F.; Polenta, G.; Puget, J-l; Rachen, J. P.; Reinecke, M.; Remazeilles, M.; Renzi, A.; Rocha, G.; Roudier, G.; Ruiz-granados, B.; Savelainen, M.; Scott, D.; Sirri, G.; Spencer, L. D.; Suur-uski, A-s; Tauber, J. A.; Tavagnacco, D.; Tenti, M.; Toffolatti, L.; Tomasi, M.; Trombetti, T.; Valiviita, J.; Van Tent, B.; Vielva, P.; Villa, F.; Wehus, I. K.; Zacchei, A.; Zonca, A.. |
| We describe an extension of the most recent version of the Planck Catalogue of Compact Sources (PCCS2), produced using a new multi-band Bayesian Extraction and Estimation Package (BeeP). BeeP assumes that the compact sources present in PCCS2 at 857 GHz have a dust-like spectral energy distribution (SED), which leads to emission at both lower and higher frequencies, and adjusts the parameters of the source and its SED to fit the emission observed in Planck's three highest frequency channels at 353, 545, and 857 GHz, as well as the IRIS map at 3000 GHz. In order to reduce confusion regarding diffuse cirrus emission, BeeP's data model includes a description of the background emission surrounding each source, and it adjusts the confidence in the source... |
| Tipo: Text |
Palavras-chave: Catalogs; Cosmology: observations; Submillimeter: general. |
| Ano: 2020 |
URL: https://archimer.ifremer.fr/doc/00666/77840/80013.pdf |
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