Power asymmetries in the cosmic microwave background temperature and polarization patterns

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 1, 2010, Pages 399-404

  Paci, F ^a   Gruppuso, A ^b,c   Finelli, F ^b,c   Cabella, P ^d   De Rosa, A ^b   Mandolesi, N ^b   Natoli, P ^d,e  

^a INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^b OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c INFN SEZIONE DI BOLOGNA   (Italy)

^d UNIVERSITY OF ROME TOR VERGATA   (Italy)

^e INFN SEZIONE DI ROMA TOR VERGATA   (Italy)

Author keywords

Cosmic microwave background; Cosmology: observations; Cosmology: theory; Methods: numerical; Methods: statistical

Indexed keywords

ANISOTROPY; COSMOLOGY; INTELLIGENT SYSTEMS; MICROWAVES; MONTE CARLO METHODS; NUMERICAL METHODS; POLARIZATION;

BACKGROUND TEMPERATURE; COSMIC MICROWAVES BACKGROUND; COSMOLOGY OBSERVATIONS; COSMOLOGY: THEORY; METHOD: NUMERICAL; METHODS:STATISTICAL; MULTIPOLES; POLARIZATION PATTERNS; POWER; POWER-SPECTRA;

POWER SPECTRUM;

EID: 77956399256     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16905.x     Document Type: Article

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