CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics

Monthly Notices of the Royal Astronomical Society

Volumn 449, Issue 2, 2015, Pages 1505-1525

  Simon, P ^a   Semboloni, E ^b,c   van Waerbeke, L ^b   Hoekstra, H ^c   Erben, T ^a   Fu, L ^d   Harnois Deraps J ^b,e   Heymans, C ^f   Hildebrandt, H ^a   Kilbinger, M ^g,h   Kitching, T D ⁱ   Miller, L ^j   Schrabback, T ^a  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^c LEIDEN UNIVERSITY   (Netherlands)

^d SHANGHAI NORMAL UNIVERSITY   (China)

^e UNIVERSITY OF TORONTO   (Canada)

^f UNIVERSITY OF EDINBURGH   (United Kingdom)

^g INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^h CEA SACLAY   (France)

ⁱ UNIVERSITY COLLEGE LONDON   (United Kingdom)

^j UNIVERSITY OF OXFORD   (United Kingdom)

more..

Author keywords

Cosmology: observations; Dark matter; Gravitational lensing: weak; Methods: statistical

Indexed keywords

COSMOLOGY; GALAXIES; GAUSSIAN DISTRIBUTION; GAUSSIAN NOISE (ELECTRONIC); GRAVITATION; OPTICAL TRANSFER FUNCTION;

BISPECTRA; COSMIC SHEAR; COSMOLOGICAL PARAMETERS; COSMOLOGY OBSERVATIONS; DARK MATTER; GAUSSIANS; GRAVITATIONAL LENSING: WEAK; LENSING SURVEY; METHODS:STATISTICAL; THIRD ORDER;

SURVEYS;

EID: 84934882568     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stv339     Document Type: Article

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