Related references
Note: Only part of the references are listed.Evidence of the accelerated expansion of the Universe from weak lensing tomography with COSMOS
T. Schrabback et al.
ASTRONOMY & ASTROPHYSICS (2010)
FROM FINANCE TO COSMOLOGY: THE COPULA OF LARGE-SCALE STRUCTURE
Robert J. Scherrer et al.
ASTROPHYSICAL JOURNAL LETTERS (2010)
Constructing a bivariate distribution function with given marginals and correlation: application to the galaxy luminosity function
Tsutomu T. Takeuchi
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)
The non-Gaussianity of the cosmic shear likelihood or how odd is the Chandra Deep Field South?
J. Hartlap et al.
ASTRONOMY & ASTROPHYSICS (2009)
SIMULATIONS OF BARYON ACOUSTIC OSCILLATIONS. II. COVARIANCE MATRIX OF THE MATTER POWER SPECTRUM
Ryuichi Takahashi et al.
ASTROPHYSICAL JOURNAL (2009)
SIMULATIONS OF WIDE-FIELD WEAK LENSING SURVEYS. I. BASIC STATISTICS AND NON-GAUSSIAN EFFECTS
Masanori Sato et al.
ASTROPHYSICAL JOURNAL (2009)
The impact of non-Gaussian errors on weak lensing surveys
Masahiro Takada et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Constraints on neutrino masses from weak lensing
Kiyotomo Ichiki et al.
PHYSICAL REVIEW D (2009)
Very weak lensing in the CFHTLS wide:: cosmology from cosmic shear in the linear regime
L. Fu et al.
ASTRONOMY & ASTROPHYSICS (2008)
Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Implications for cosmology
D. N. Spergel et al.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2007)
Dark energy constraints from the CTIO lensing survey
Mike Jarvis et al.
ASTROPHYSICAL JOURNAL (2006)
Cosmic shear analysis with CFHTLS deep data
E. Semboloni et al.
ASTRONOMY & ASTROPHYSICS (2006)
Stable clustering, the halo model and non-linear cosmological power spectra
RE Smith et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)
Cosmic shear statistics in the Suprime-Cam 2.1 square degree field: Constraints on Omega(m) and sigma(8)
T Hamana et al.
ASTROPHYSICAL JOURNAL (2003)
Cosmological parameters from CMB and other data: A Monte Carlo approach
A Lewis et al.
PHYSICAL REVIEW D (2002)
Share Paper
