Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum

Monthly Notices of the Royal Astronomical Society

Volumn 455, Issue 3, 2016, Pages 2573-2581

  Kalus, B ^a   Percival, W J ^a   Samushia, L ^a,b,c  

^a UNIVERSITY OF PORTSMOUTH   (United Kingdom)

^b KANSAS STATE UNIVERSITY   (United States)

^c ILIA STATE UNIVERSITY   (Georgia)

Author keywords

Inflation; Large scale structure of Universe; Methods: statistical

Indexed keywords

COVARIANCE MATRIX; GALAXIES; GAUSSIAN DISTRIBUTION; SURVEYS;

COSMOLOGICAL PARAMETERS; COVARIANCE MATRICES; GALAXY CLUSTERING; GAUSSIANS; INFLATION; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:STATISTICAL; PARAMETER INFERENCE; POSTERIOR DISTRIBUTIONS; POWER-SPECTRA;

POWER SPECTRUM;

EID: 84959123174     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stv2307     Document Type: Article

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