Planck intermediate results

The six parameters of the standard ΛCDM model have best-fit values derived from the Planck temperature power spectrum that are shifted somewhat from the best-fit values derived from WMAP data. These shifts are driven by features in the Planck temperature power spectrum at angular scales that had nev...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2017-11, Vol.607
Hauptverfasser:	Ashdown, M., Aumont, J., Baccigalupi, C., Benabed, K., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Calabrese, E., Cardoso, J.-F., Challinor, A., Chiang, H. C., Colombo, L. P. L., Combet, C., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Ducout, A., Dupac, X., Dusini, S., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fantaye, Y., Finelli, F., Frailis, M., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., Gratton, S., Gruppuso, A., Gudmundsson, J. E., Jaffe, A. H., Jones, W. C., Keihänen, E., Keskitalo, R., Kim, J., Kisner, T. S., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lawrence, C. R., Le Jeune, M., Lewis, A., Liguori, M., Lilje, P. B., Lindholm, V., López-Caniego, M., Lubin, P. M., Maino, D., Mandolesi, N., Martin, P. G., McEwen, J. D., Meinhold, P. R., Migliaccio, M., Millea, M., Miville-Deschênes, M.-A., Molinari, D., Morgante, G., Moss, A., Narimani, A., Natoli, P., Paoletti, D., Partridge, B., Patanchon, G., Pettorino, V., Polastri, L., Puget, J.-L., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rossetti, M., Ruiz-Granados, B., Salvati, L., Savelainen, M., Sirri, G., Stanco, L., Suur-Uski, A.-S., Tavagnacco, D., Tenti, M., Toffolatti, L., Tristram, M., Trombetti, T., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., White, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Computer simulation cosmic background radiation cosmological parameters cosmology: observations cosmology: theory Datasets Density Gravitational effects Gravitational lenses Intergalactic media Mathematical models Optical analysis Parameters Sample variance South Pole Temperature Thermal energy
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