Browsing by Author "Bond, J. R."

Now showing items 1-4 of 4

    • Dust-correlated cm wavelength continuum emission from translucent clouds ζ Oph and LDN 1780 
      Vidal, M.; Casassus Montero, Simón; Dickinson, C.; Witt, A. N.; Castellanos, P.; Davies, R. D.; Davis, R. J.; Cabrera, G.; Cleary, K.; Allison, J. R.; Bond, J. R.; Bronfman Aguiló, Leonardo; Bustos, R.; Jones, M. E.; Paladini, R.; Pearson, T. J.; Readhead, A. C. S.; Reeves, R.; Sievers, J. L.; Taylor, A. C. (2011)
      The diffuse cm wave IR-correlated signal, the ‘anomalous’ CMB foreground, is thought to arise in the dust in cirrus clouds.We present Cosmic Background Imager (CBI) cm wave data of two translucent clouds, ζ Oph and LDN ...
    • Extended mosaic observations with the Cosmic Background Imager 
      Readhead, A. C. S.; Mason, B. S.; Contaldi, C. R.; Pearson, T. J.; Bond, J. R.; Myers, S. T.; Padin, S.; Sievers, J. L.; Cartwright, J. K.; Shepherd, M. C.; Pogosyan, D.; Prunet, S.; Altamirano, P.; Bustos, R.; Bronfman Aguiló, Leonardo; Casassus Montero, Simón; Holzapfel, W. L.; May Humeres, Jorge; Pen, U.-L.; Torres, S.; Udomprasert, P. S. (IOP PUBLISHING, 2004-07-10)
      Two years of microwave background observations with the Cosmic Background Imager ( CBI) have been combined to give a sensitive, high-resolution angular power spectrum over the range 400 < l < 3500. This power spectrum has ...
    • Implications of the cosmic background imager polarization data 
      Sievers, J. L.; Achermann, C.; Bond, J. R.; Bronfman Aguiló, Leonardo; Bustos, R.; Contaldi, C. R.; Dickinson, C.; Ferreira, P. G.; Jones, M. E.; Lewis, A. M.; Mason, B. S.; May Humeres, Jorge; Myers, S. T.; Oyarce, N.; Padin, S.; Pearson, T. J.; Pospieszalski, M.; Readhead, A. C. S.; Reeves, R.; Taylor, A. C.; Torres, S. (2007)
      We present new measurements of the power spectra of the E mode of cosmic microwave background (CMB) polarization, the temperature T, the cross-correlation of E and T, and upper limits on the B mode from 2.5 yr of dedicated ...
    • Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae 
      Arnaud, M.; Atrio-Barandela, F.; Aumont, J.; Baccigalupi, C.; Banday, A.; Barreiro, R.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bernard, J. P.; Bersanelli, M.; Bielewicz, P.; Bonaldi, A.; Bond, J. R.; Borrill, J.; Bouchet, F.; Buemi, C. S.; Burigana, C.; Cardoso, J.; Casassus Montero, Simón; Catalano, A.; Cerrigone, L.; Chamballu, A.; Chiang, H.; Colombi, S.; Colombo, L.; Couchot, F.; Crill, B.; Curto, A.; Cuttaia, F.; Davies, R. D.; Davis, R. J.; Bernardis, P. de; Rosa, A. de; Zotti, G. de; Delabrouille, J.; Dickinson, C.; Diego, J.; Donzelli, S.; Doré, O.; Dupac, X.; Enblin, T. A.; Eriksen, H. K.; Finelli, F.; Frailis, M.; Franceschi, E.; Galeotta, S.; Ganga, K.; Giard, M.; González-Nuevo, J.; Górski, K.; Gregorio, A.; Gruppuso, A.; Hansen, F.; Harrison, D.; Hildebrandt, S. R.; Hivon, E.; Holmes, W.; Hora, J. L.; Hornstrup, A.; Hovest, W.; Huffenberger, K. M.; Jaffe, T.; Jones, W.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kisner, T.; Knoche, J.; Kunz, M.; Kurki-Suonio, H.; Lähteenmäki, A.; Lamarre, J.-M.; Lasenby, A.; Lawrence, C. R.; Leonardi, R.; Leto, P.; Lilje, P.; Linden-Vornle, M.; López-Caniego, M.; Macías-Pérez, J.; Maffei, B.; Maino, D.; Mandolesi, N.; Martin, P. G.; Masi, S.; Massardi, M.; Matarrese, S.; Mazzotta, P.; Mendes, L.; Mennella, A.; Migliaccio, M.; Miville-Deschênes, M.-A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Munshi, D.; Murphy, J.; Naselsky, P.; Nati, F.; Natoli, P.; Noviello, F.; Novikov, D.; Novikov, I.; Pagano, L.; Pajot, F.; Paladini, R.; Paoletti, D.; Peel, Murray C.; Perdereau, O.; Perrotta, F.; Piacentini, F.; Piat, M.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Popa, L.; Pratt, G. W.; Procopio, P.; Prunet, S.; Puget, J.-L.; Rachen, J.; Reinecke, M.; Remazeilles, M.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Roudier, G.; Rubiño-Martín, J.; Rusholme, B.; Sandri, M.; Savini., G.; Scott, D.; Spencer, L.; Stolyarov, V.; Sutton, D.; Suur-Uski, A.-S.; Sygnet, J.; Tauber, J. A.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Trigilio, C.; Tristram, M.; Trombetti, T.; Tucci, M.; Umana, G.; Valiviita, J.; Van Tent, B.; Vielva, P.; Villa, F.; Wade, L.; Wandelt, B.; Zacchei, A.; Zijlstra, A.; Zonca, A. (EDP Sciences, 2015)
      Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on ...