The expansion of the universe causes spacetime curvature, distinguishing between distances measured along and transverse to the line of sight. The ratio of these distances, e.g. the cosmic shear distortion of a sphere defined by observations of large scale structure as suggested by Alcock & Paczynski, provides a method for exploring the expansion as a function of redshift. The theoretical sensitivity to cosmological parameters, including the dark energy equation of state, is presented. Remarkably, sensitivity to the time variation of the dark energy equation of state is best achieved by observations at redshifts z<1. While systematic errors greatly degrade the theoretical sensitivity, this probe may still offer useful parameter estimation, ...
The current cosmological concordance model, ΛCDM, is very successful at describing the statistical p...
Massive redshift surveys of galaxies beyond the local Universe (i.e. z > 0.3) provide an exhausti...
We adapt the Jain--Taylor (2003) shear-ratio geometric lensing method to measure the dark energy equ...
One of the principal goals of modern cosmology is to constrain the properties of dark energy. At pre...
Measurements of the growth rate of structure f at different redshifts can discriminate the origin of...
We review the ability of redshift surveys to provide constraints on the Dark Energy content of the U...
Abstract. Cosmic shear surveys are now collecting photometric redshifts of the sources. We analyse h...
One PDF file including both main paper and Supplementary Information (28 pages, 3+2 figures). Publis...
bservations of distant supernovae indicate that the Universe is now in a phase of accelerated expans...
The cosmological interpretation of weak lensing by large-scale structures requires knowledge of the ...
Gravitational lensing can provide pure geometric tests of the structure of spacetime, for instance b...
The variation of the expansion rate of the Universe with time produces an evolution in the cosmologi...
International audienceGravitational lensing can provide pure geometric tests of the structure of spa...
The current cosmological concordance model, ΛCDM, is very successful at describing the statistical p...
Massive redshift surveys of galaxies beyond the local Universe (i.e. z > 0.3) provide an exhausti...
We adapt the Jain--Taylor (2003) shear-ratio geometric lensing method to measure the dark energy equ...
One of the principal goals of modern cosmology is to constrain the properties of dark energy. At pre...
Measurements of the growth rate of structure f at different redshifts can discriminate the origin of...
We review the ability of redshift surveys to provide constraints on the Dark Energy content of the U...
Abstract. Cosmic shear surveys are now collecting photometric redshifts of the sources. We analyse h...
One PDF file including both main paper and Supplementary Information (28 pages, 3+2 figures). Publis...
bservations of distant supernovae indicate that the Universe is now in a phase of accelerated expans...
The cosmological interpretation of weak lensing by large-scale structures requires knowledge of the ...
Gravitational lensing can provide pure geometric tests of the structure of spacetime, for instance b...
The variation of the expansion rate of the Universe with time produces an evolution in the cosmologi...
International audienceGravitational lensing can provide pure geometric tests of the structure of spa...
The current cosmological concordance model, ΛCDM, is very successful at describing the statistical p...
Massive redshift surveys of galaxies beyond the local Universe (i.e. z > 0.3) provide an exhausti...
We adapt the Jain--Taylor (2003) shear-ratio geometric lensing method to measure the dark energy equ...