The integrated bispectrum as a test of cosmic microwave background non-Gaussianity: Detection power and limits on fNL with WMAP data

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 2, 2006, Pages 819-824

  Cabella, P ^a   Hansen, F K ^b   Liguori, M ^c,d,e   Marinucci, D ^f   Matarrese, S ^d,e   Moscardini, L ^g   Vittorio, N ^f,h  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b UNIVERSITY OF OSLO   (Norway)

^c FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^d UNIVERSITY OF PADOVA   (Italy)

^e SEZIONE DI PADOVA   (Italy)

^f UNIVERSITY OF ROME TOR VERGATA   (Italy)

^g UNIVERSITY OF BOLOGNA   (Italy)

^h INFN SEZIONE DI ROMA TOR VERGATA   (Italy)

Author keywords

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

Indexed keywords

COMPUTATION THEORY; GAUSSIAN NOISE (ELECTRONIC); NUMERICAL METHODS;

BISPECTRA; COSMIC MICROWAVES BACKGROUND; COSMOLOGY OBSERVATIONS; COSMOLOGY: THEORY; DETECTION POWER; METHOD: NUMERICAL; METHODS:STATISTICAL; MULTIPOLES; NONGAUSSIAN SIGNALS; NONGAUSSIANITY;

COSMOLOGY;

EID: 33744949481     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10339.x     Document Type: Article

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