Simulation of non-Gaussian cosmic microwave background maps

Monthly Notices of the Royal Astronomical Society

Volumn 357, Issue 1, 2005, Pages 1-11

  Rocha, Graca ^a,b,c   Hobson, M P ^a   Smith, Sarah ^a   Ferreira, Pedro ^b   Challinor, Anthony ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c CENTRO DE ASTROFÍSICA   (Portugal)

Author keywords

Cosmic microwave background; Cosmology: Theory; Methods: Statistical

Indexed keywords

CORRELATORS; COSMOLOGY; GAUSSIAN DISTRIBUTION; PIXELS; POWER SPECTRUM; PROBABILITY DENSITY FUNCTION;

BISPECTRA; COSMIC MICROWAVES BACKGROUND; COSMOLOGY: THEORY; GAUSSIAN MAP; METHODS:STATISTICAL; NON-GAUSSIAN; NON-GAUSSIAN DISTRIBUTION; PIXEL VALUES; POWER-SPECTRA; SIMPLE METHOD;

GAUSSIAN NOISE (ELECTRONIC);

EID: 13744260797     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08552.x     Document Type: Article

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