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1“... models, on CMB anisotropies are investigated. Late-time reionization reduces the CMB anisotropies...”
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2“... directions of the clusters can point to a cosmic ray anisotropy. As a result of analysis of clusters...”
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4by Benoît, A“... microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived as a...”
Published 2002
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6“...We report on additional observations of degree scale anisotropy at 90~GHz from the Amundsen-Scott...”
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7“... on the cosmic microwave background anisotropies. More specifically, we computed the \dtt corresponding...”
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8by Peterson, J B, Griffin, G S, Newcomb, M G, Alvarez, D L, Cantaloupo, C, Morgan, D, Miller, K W, Ganga, K, Pernic, D, Thoma, M H“...Results of a search for small-scale anisotropy in the cosmic microwave background (CMB...”
Published 1999
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9“...We use Owens Valley Radio Observatory (OVRO) cosmic microwave background (CMB) anisotropy data...”
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10“...We use data from the ARGO cosmic microwave background (CMB) anisotropy experiment to constrain...”
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11by Coble, K A“.... Interpreting the observed fluctuations as anisotropy in the cosmic microwave background, we place constraints...”
Published 1999
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12by Coble, K, Dragovan, M, Kovács, J, Halverson, N W, Holzapfel, W L, Knox, L, Dodelson, S, Ganga, K, Alvarez, D, Peterson, J B, Griffin, G, Newcomb, M, Miller, K, Platt, S R, Novák, G S“... fluctuations as anisotropy in the cosmic microwave background, we place constraints on the angular power...”
Published 1999
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13by Mukherjee, P, Coble, K, Dragovan, M, Ganga, K, Kovács, J M, Ratra, B, Souradeep, T“... anisotropy data by cross correlating it with foreground contaminant emission templates. To model foreground...”
Published 2003
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14“...) temperature anisotropies at high angular resolution (8 arcminutes) over a large fraction (25%) of the sky...”
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15“... microwave background (CMB) anisotropy data by cross-correlating with templates of infrared dust emission...”
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16by Désert, F X“..., and is almost perfectly isotropic, the anisotropies being about one part to 100,000. However, these anisotropies...”
Published 2001
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17“...We use Python I, II, and III cosmic microwave background anisotropy data to constrain cosmogonies...”
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18“... microwave background (CMB) anisotropy data from the MAX 4 and MAX 5 experiments. These analyses use CMB...”
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19“...We analyze the 1994 UCSB South Pole CMB anisotropy data in the context of realistic open and flat...”
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20by Crill, B P, Ade, P A R, Artusa, D R, Bhatia, R S, Bock, J J, Boscaleri, A, Cardoni, P, Church, S E, Coble, K, De Bernardis, P, De Troia, G, Farese, P, Ganga, K, Giacometti, M, Haynes, C V, Hivon, E, Hristov, V V, Iacoangeli, A, Jones, W C, Lange, A E, Martinis, L, Masi, S, Mason, P V, Mauskopf, P D, Miglio, L, Montroy, T, Netterfield, C B, Paine, C G, Pascale, E, Piacentini, F, Pongetti, F, Romeo, G, Ruhl, J E, Scaramuzzi, F, Sforza, D M, Turner, A D“... filters, and cryogenics to obtain high sensitivity to CMB anisotropy. Sixteen detectors observe in 4...”
Published 2002
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