Fast optimal CMB power spectrum estimation with Hamiltonian sampling

Monthly Notices of the Royal Astronomical Society

Volumn 389, Issue 3, 2008, Pages 1284-1292

  Taylor, J F ^a   Ashdown, M A J ^a   Hobson, M P ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Cosmic microwave background; Methods: data analysis; Methods: statistical

Indexed keywords

HAMILTONIANS; POWER SPECTRUM; PROBABILITY DISTRIBUTIONS; SAMPLING; SIGNAL TO NOISE RATIO; SPECTRUM ANALYSIS;

ANGULAR POWER SPECTRUM; CORRELATION LENGTHS; COSMIC MICROWAVES BACKGROUND; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; OPTIMAL ESTIMATIONS; POSTERIOR PROBABILITY; POWER SPECTRUM ESTIMATION; SIGNAL TO NOISE; WILKINSON MICROWAVE ANISOTROPY PROBE;

COSMOLOGY;

EID: 51349108375     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13630.x     Document Type: Article

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