New estimates of the CMB angular power spectra from the WMAP 5 year low-resolution data

Monthly Notices of the Royal Astronomical Society

Volumn 400, Issue 1, 2009, Pages 463-469

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

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b INFN SEZIONE DI BOLOGNA   (Italy)

^c UNIVERSITY OF ROME TOR VERGATA   (Italy)

^d UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

^e UNIVERSITY OF BOLOGNA   (Italy)

^f INFN SEZIONE DI ROMA TOR VERGATA   (Italy)

Author keywords

Cosmic microwave background; Cosmology: Observations; Cosmology: Theory; Methods: Numerical; Methods: Statistical

Indexed keywords

CODES (SYMBOLS); COMPUTATION THEORY; COVARIANCE MATRIX; MAXIMUM LIKELIHOOD ESTIMATION; NUMERICAL METHODS; POWER SPECTRUM;

ANGULAR POWER SPECTRUM; CONDITIONAL LIKELIHOOD; COSMIC MICROWAVES BACKGROUND; COSMOLOGY OBSERVATIONS; COSMOLOGY: THEORY; ERROR BARS; METHOD: NUMERICAL; METHODS:STATISTICAL; POWER-SPECTRA; WILKINSON MICROWAVE ANISOTROPY PROBE;

COSMOLOGY;

EID: 70449555378     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15469.x     Document Type: Article

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