Model selection as a science driver for dark energy surveys

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 4, 2006, Pages 1725-1734

  Mukherjee, Pia ^a   Parkinson, David ^a   Corasaniti, Pier Stefano ^b   Liddle, Andrew R ^a   Kunz, Martin ^c  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b Columbia University ^*  (United States)

^c UNIVERSITY OF GENEVA   (Switzerland)

Author keywords

Cosmological parameters; Cosmology: theory; Methods: statistical

Indexed keywords

BAYESIAN NETWORKS; COSMOLOGY; SURVEYS;

BAYES FACTOR; COSMOLOGICAL PARAMETERS; COSMOLOGY: THEORY; DARK ENERGY; ENERGY SURVEYS; METHODS:STATISTICAL; MODEL SELECTION; POWER; SEEK TIME; TIME EVOLUTIONS;

SUPERNOVAE;

EID: 33745541350     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10427.x     Document Type: Article

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