Browsing by Subject "Cosmic microwave background"

Now showing items 1-5 of 5

    • A Measurement of the CMB E-mode Angular Power Spectrum at Subdegree Scales from 670 Square Degrees of ... 
      Adachi, S.; Aguilar Faúndez, M. A. O.; Arnold, K.; Baccigalupi, C.; Barron, D.; Beck, D.; Bianchini, F.; Chapman, S.; Cheung, K.; Chinone, Y.; Crowley, K.; Dobbs, M.; El-Bouhargani, H.; Elleflot, T.; Errard, J.; Fabbian, G.; Feng, C.; Fujino, T.; Galitzki, N.; Goeckner Wald, N.; Groh, J.; Hall, G.; Hasegawa, M.; Hazumi, M.; Hirose, H.; Jaffe, A. H.; Jeong, O; Kaneko, D.; Katayama, N.; Keating, B.; Kikuchi, S.; Kisner, T.; Kusaka, A.; Lee, A. T.; León, D.; Linder, E.; Lowry, L. N.; Matsuda, F.; Matsumura, T.; Minami, Y.; Navaroli, M.; Nishino, H.; Pham, A. T. P.; Poletti, D.; Reichardt, C. L.; Segawa, Y.; Siritanasak, P.; Tajima, O.; Takakura, S.; Takatori, S.; Tanabe, D.; Tsai, C.; Verges, C.; Westbrook, B.; Zhou, Y. (IOP, 2020)
      We report a measurement of the E-mode polarization power spectrum of the cosmic microwave background (CMB) using 150 GHz data taken from 2014 July to 2016 December with the POLARBEAR experiment. We reach an effective ...
    • Progress Report on the Large‑Scale Polarization Explorer 
      Lamagna, L.; Addamo, G.; Ade, P. A. R.; Baccigalupi, C.; Baldini, A.M.; Battaglia, P.M.; Battistelli, E.; Bau, A.; Bersanelli, M.; Biasotti, M.; Boscaleri; Boragno, C.; Boscaleri, A.; Caccianiga, B.; Caprioli, S.; Cavaliere, F.; Cei, F.; Cleary, K.A.; Columbro, F.; Coppi, G.; Coppolecchia, A.; Corsini, D.; Cuttaia, F.; D'Alessandro, G.; Bernardis, P. de; De Gasperis, G.; De Petris, M.; Torto, F. del; Fafone, V.; Farooqui, Z.; Farsian, F.; Fontanelli, F.; Franceschet, C.; Gaier, T.C.; Gatti, F.; Genova-Santos, R.; Gervasi, M.; Ghigna, T.; Grassi, M.; Grosso, D.; Incardona, F.; Jones, M.; Kangaslahti, P.; Krachmalnicoff, N.; Mainini, R.; Maino, D.; Mandelli, S.; Maris, M.; Masi, S.; Matarrese, S.; May, A.; Mena, P.; Mennella, A.; Molina, R.; Molinari, D.; Morgante, G.; Nati, F.; Natoli, P.; Pagano, L.; Paiella, A.; Paonessa, F.; Passerini, A.; Perez-de-Taoro, M.; Peverini, O.A.; Pezzotta, F.; Piacentini, F.; Piccirillo, L.; Pisano, G.; Polastri, L.; Polenta, G.; Poletti, D.; Presta, G.; Realini, S.; Reyes, N.; Rocchi, A.; Rubino Martin, J. A.; Sandri, M.; Sartor, S.; Schillaci, A.; Signorelli, G.; Soria, M.; Spinella, F.; Tapia, V.; Tartari, A.; Taylor, A.; Terenzi, L.; Tomasi, M.; Tommasi, E.; Tucker, C.; Vaccaro, D.; Vigano, D.M.,; Villa, F.; Virone, G.; Vittorio, N.; Volpe, A.; Watkins, B.; Zacchei, A.; Zannoni, M. (Springer, 2020)
      The large-scale polarization explorer (LSPE) is a cosmology program for the measurement of large-scale curl-like features (B-modes) in the polarization of the cosmic microwave background. Its goal is to constrain the ...
    • The anisotropy of the microwave background to l = 3500: Deep field observations with the cosmic background imager 
      Mason, B. S.; Pearson, T. J.; Readhead, A. C.S.; Shepherd, M. C.; Sievers, J.; Udomprasert, P. S.; Cartwright, J. K.; Farmer, A. J.; Padin, S.; Myers, S. T.; Bond, J. R.; Contaldi, C. R.; Pen, U.; Prunet, S.; Pogosyan, D.; Carlstrom, J. E.; Kovac, J.; Leitch, E. M.; Pryke. C.; Halverson, N.W.; Holzapfel, W. L.; Altamirano, P.; Bronfman Aguiló, Leonardo; Casassus Montero, Simón; May, J.; Joy, M. (Institute of Physics Publishing, 2003)
      We report measurements of anisotropy in the cosmic microwave background radiation over the multipole range l ∼ 200-3500 with the Cosmic Background Imager based on deep observations of three fields. These results confirm ...
    • The anisotropy of the microwave background to l = 3500: Mosaic observations with the cosmic background imager 
      Pearson, T. J.; Mason, B. S.; Readhead, A. C.S.; Shepherd, M. C.; Sievers, J. L.; Udomprasert, P. S.; Cartwright, J. K.; Farmer, A. J.; Padin, S.; Myers, S. T.; Bond, J. R.; Contaldi, C. R.; Pen, U. L.; Prunet, S.; Pogosyan, D.; Carlstrom, J. E.; Kovac, J.; Leitch, E. M.; Pryke. C.; Halverson, N. W.; Holzapfel, W. L.; Altamirano, P.; Bronfman Aguiló, Leonardo; Casassus Montero, Simón; May, J.; Joy, M. (Institute of Physics Publishing, 2003)
      Using the Cosmic Background Imager (CBI), a 13-element interferometer array operating in the 26-36 GHz frequency band, we have observed 40 deg 2 of sky in three pairs of fields, each ∼1457prime; × 165′, using overlapping ...
    • 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. ...