Browsing by Author "Paladini, R."

Now showing items 1-5 of 5

    • Constraints on free–free emission from anomalous microwave emission sources in the perseus molecular cloud 
      Tibbs, C.; Paladini, R.; Dickinson, C.; Mason, B.S.; Casassus Montero, Simón; Cleary, K.; Davies, R.D.; Davis, R.J.; Watson, R.A. (The American Astronomical Society, 2013-06-20)
      We present observations performed with the Green Bank Telescope at 1.4 and 5 GHz of three strips coincident with the anomalous microwave emission features previously identified in the Perseus molecular cloud at 33 GHz ...
    • 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 ...
    • 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 ...
    • Spitzer characterization of dust in an anomalous emission region: the Perseus cloud 
      Tibbs, C. T.; Flagey, N.; Paladini, R.; Compiègne, M.; Shenoy, S.; Carey, S.; Noriega Crespo, A.; Dickinson, C.; Ali Haïmoud, Y.; Casassus Montero, Simón; Cleary, K.; Davies, R. D.; Hirata, C. M.; Watson, R. A. (2011)
      Anomalous microwave emission is known to exist in the Perseus cloud. One of the most promising candidates to explain this excess of emission is electric dipole radiation from rapidly rotating very small dust grains, ...
    • The State-of-Play of Anomalous Microwave Emission (AME) research 
      Dickinson, Clive; Ali-Haïmoud, Y.; Barr, A.; Battistelli, E.; Bell, A.; Bernstein, L.; Casassus Montero, Simón; Cleary, K.; Draine, B.; Génova-Santos, R.; Harper, S.; Hensley, B.; Hill-Valler, J.; Hoang, Thiem; Israel, F.; Jew, L.; Lazarian, A.; Leahy, J.; Leech, J.; López-Caraballo, C.; McDonald, I.; Murphy, E.; Onaka, T.; Paladini, R.; Peel, M.; Perrott, Y.; Poidevin, F.; Readhead, A.; Rubiño-Martín, J.; Taylor, A.; Tibbs, C.; Todorović, M.; Vidal, Matías (Elsevier B.V., 2018)
      Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997. ...