In paper I (Yu et al. [1]), we showed through N-body simulation that a local monotonic Gaussian transformation can significantly reduce non-Gaussianity in a noise-free lensing convergence field. This makes the Gaussianization a promising theoretical tool to understand high-order lensing statistics. Here we present a study of its applicability in lensing data analysis, in particular when shape measurement noise is presented in lensing convergence maps. (i) We find that shape measurement noise significantly degrades the Gaussianization performance and the degradation increases for shallower surveys. (ii) The Wiener filter is efficient in reducing the impact of shape measurement noise. The Gaussianization of the Wiener-filtered lensing maps is...
International audienceWe study the morphology of convergence maps by perturbatively reconstructing t...
none7While usually cosmological initial conditions are assumed to be Gaussian, inflationary theories...
We implement the Elliptical Gauss-Laguerre (EGL) galaxy-shape measurement method proposed by Bernste...
Motivated by recent works of Neyrinck et al. 2009 and Scherrer et al. 2010, we proposed a Gaussian t...
Taking into account the noise from intrinsic ellipticities of source galaxies, we study the efficien...
Abstract Taking into account the noise from intrinsic ellipticities of source galaxies, we study the...
Weak lensing experiments are a powerful probe into cosmology through their measurement of the mass d...
Mapping the underlying density field, including non-visible dark matter, using weak gravitational le...
Mapping the underlying density field, including non-visible dark matter, using weak gravitational le...
International audienceMapping the underlying density field, including non-visible dark matter, using...
Weak gravitational lensing has become a common tool to constrain the cosmological model. The majorit...
The power spectrum of weak lensing fluctuations has a non-Gaussian distribution due to its quadratic...
<p>The robust estimation of the tiny distortions (shears) of galaxy shapes caused by weak gravitatio...
We apply an analytic method to predict peak counts in weak-lensing surveys. It is based on the theo...
International audienceWe investigate the accuracy of weak lensing simulations by comparing the resul...
International audienceWe study the morphology of convergence maps by perturbatively reconstructing t...
none7While usually cosmological initial conditions are assumed to be Gaussian, inflationary theories...
We implement the Elliptical Gauss-Laguerre (EGL) galaxy-shape measurement method proposed by Bernste...
Motivated by recent works of Neyrinck et al. 2009 and Scherrer et al. 2010, we proposed a Gaussian t...
Taking into account the noise from intrinsic ellipticities of source galaxies, we study the efficien...
Abstract Taking into account the noise from intrinsic ellipticities of source galaxies, we study the...
Weak lensing experiments are a powerful probe into cosmology through their measurement of the mass d...
Mapping the underlying density field, including non-visible dark matter, using weak gravitational le...
Mapping the underlying density field, including non-visible dark matter, using weak gravitational le...
International audienceMapping the underlying density field, including non-visible dark matter, using...
Weak gravitational lensing has become a common tool to constrain the cosmological model. The majorit...
The power spectrum of weak lensing fluctuations has a non-Gaussian distribution due to its quadratic...
<p>The robust estimation of the tiny distortions (shears) of galaxy shapes caused by weak gravitatio...
We apply an analytic method to predict peak counts in weak-lensing surveys. It is based on the theo...
International audienceWe investigate the accuracy of weak lensing simulations by comparing the resul...
International audienceWe study the morphology of convergence maps by perturbatively reconstructing t...
none7While usually cosmological initial conditions are assumed to be Gaussian, inflationary theories...
We implement the Elliptical Gauss-Laguerre (EGL) galaxy-shape measurement method proposed by Bernste...