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Ade, Peter;Aghanim, N.;Arnaud, M.;Ashdown, M.;Aubourg, E.;Aumont, J.;Baccigalupi, C.;Banday, A. J.;Barreiro, R. B.;Bartolo, N.;Battaner, E.;Benabed, K.;Benoit-Lévy, A.;Bersanelli, M.;Bielewicz, P.;Bock, J. J.;Bonaldi, A.;Bonavera, L.;Bond, J. R.;Borrill, J.;Bouchet, F. R.;Burigana, C.;Calabrese, Erminia;Cardoso, J.-F.;Catalano, A.;Chamballu, A.;Chiang, H. C.;Christensen, P. R.;Clements, D. L.;Colombo, L. P. L.;Combet, C.;Crill, B. P.;Curto, A.;Cuttaia, F.;Danese, L.;Davies, R. D.;Davis, R. J.;de Bernardis, P.;de Zotti, G.;Delabrouille, J.;Dickinson, C.;Diego, J. M.;Dolag, K.;Donzelli, S.;Doré, O.;Douspis, M.;Ducout, A.;Dupac, X.;Efstathiou, G.;Elsner, F.;Enßlin, T. A.;Eriksen, H. K.;Finelli, F.;Forni, O.;Frailis, M.;Fraisse, A. A.;Franceschi, E.;Frejsel, A.;Galeotta, S.;Galli, S.;Ganga, K.;Génova-Santos, R. T.;Giard, M.;Gjerløw, E.;González-Nuevo, J.;Górski, K. M.;Gregorio, A.;Gruppuso, A.;Hansen, F. K.;Harrison, D. L.;Henrot-Versillé, S.;Hernández-Monteagudo, C.;Herranz, D.;Hildebrandt, S. R.;Hivon, E.;Hobson, M.;Hornstrup, A.;Huffenberger, K. M.;Hurier, G.;Jaffe, A. H.;Jaffe, T. R.;Jones, W. C.;Juvela, M.;Keihänen, E.;Keskitalo, R.;Kitaura, F.;Kneissl, R.;Knoche, J.;Kunz, M.;Kurki-Suonio, H.;Lagache, G.;Lamarre, J.-M.;Lasenby, A.;Lattanzi, M.;Lawrence, C. R.;Leonardi, R.;León-Tavares, J.;Levrier, F.;Liguori, M.;Lilje, P. B.;Linden-Vørnle, M.;López-Caniego, M.;Lubin, P. M.;Ma, Y.-Z.;Macías-Pérez, J. F.;Maffei, B.;Maino, D.;Mak, D. S. Y.;Mandolesi, N.;Mangilli, A.;Maris, M.;Martin, P. G.;Martínez-González, E.;Masi, S.;Matarrese, S.;McGehee, P.;Melchiorri, A.;Mennella, A.;Migliaccio, M.;Miville-Deschênes, M.-A.;Moneti, A.;Montier, L.;Morgante, G.;Mortlock, D.;Munshi, D.;Murphy, J. A.;Naselsky, P.;Nati, F.;Natoli, P.;Noviello, F.;Novikov, D.;Novikov, I.;Oxborrow, C. A.;Pagano, L.;Pajot, F.;Paoletti, D.;Perdereau, O.;Perotto, L.;Pettorino, V.;Piacentini, F.;Piat, M.;Pierpaoli, E.;Pointecouteau, E.;Polenta, G.;Ponthieu, N.;Pratt, G. W.;Puget, J.-L.;Puisieux, S.;Rachen, J. P.;Racine, B.;Reach, W. T.;Reinecke, M.;Remazeilles, M.;Renault, C.;Renzi, A.;Ristorcelli, I.;Rocha, G.;Rosset, C.;Rossetti, M.;Roudier, G.;Rubiño-Martín, J. A.;Rusholme, B.;Sandri, M.;Santos, D.;Savelainen, M.;Savini, G.;Scott, D.;Spencer, L. D.;Stolyarov, V.;Sudiwala, R.;Sunyaev, R.;Sutton, D.;Suur-Uski, A.-S.;Sygnet, J.-F.;Tauber, J. A.;Terenzi, L.;Toffolatti, L.;Tomasi, M.;Tucci, M.;Valenziano, L.;Valiviita, J.;Van Tent, B.;Vielva, P.;Villa, F.;Wade, L. A.;Wandelt, B. D.;Wang, W.;Wehus, I. K.;Yvon, D.;Zacchei, A.;Zonca, A.
By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows around central galaxies (CGs) at redshift z ≈ 0.1. We estimate the pairwise...
We present a progress report on a project to derive the evolution of the volumetric supernova Type Ia rate from the Supernova Legacy Survey. Our preliminary estimate of the rate evolution divides the sample from Neill et al. into two redshift bins: 0...
We present new techniques for improving the efficiency of supernova (SN) classification at high redshift using 64 candidates observed at Gemini North and South during the first year of the Supernova Legacy Survey (SNLS). The SNLS is an ongoing 5 year...
We use three years of data from the Supernova Legacy Survey (SNLS) to study the general properties of core-collapse and type Ia supernovae. This is the first such study using the "rolling search" technique which guarantees well-sampled SNLS light cur...
Aims. We present an empirical model of type la supernovae spectro-photometric evolution with time. Methods. The model is built using a large data set including light-curves and spectra of both nearby and distant supernovae, the latter being observed ...
We present a measurement of the distant Type la supernova (SN Ia) rate derived from the first 2 yr of the Canada-France-Hawaii Telescope Supernova Legacy Survey. We observed four 1° × 1° fields with a typical temporal frequency of (Δt) ∼ 4 observer-f...