Results 101 to 110 of about 33,635 (203)
We present results of our cosmic shear survey in progress at the Canada- France-Hawaii Telescope (CFHT). We analysed 1.7 sq. degrees of data, out of which we measured a significant correlation of galaxy shape-orientation over several arcmin scale. We present measurements of the variance of the shear $$ and of the correlation functions $$, $$.
van Waerbeke, L. +12 more
openaire +2 more sources
Accuracy requirements on intrinsic alignments for Stage-IV cosmic shear
In the context of cosmological weak lensing studies, intrinsic alignments (IAs) are one of the most In the context of cosmological weak lensing studies, intrinsic alignments (IAs) are one of the most complicated astrophysical systematic\rev{s} to model,
Anya Paopiamsap +4 more
doaj +1 more source
Cosmic shear without shape noise
We describe a new method for reducing the shape noise in weak lensing measurements by an order of magnitude. Our method relies on spectroscopic measurements of disk galaxy rotation and makes use of the Tully-Fisher relation in order to control for the intrinsic orientations of galaxy disks. For this new proposed method, so-called Kinematic Lensing (KL),
Huff, Eric M. +5 more
openaire +2 more sources
Measuring neutrino masses with a future galaxy survey
We perform a detailed forecast on how well a Euclid-like photometric galaxy and cosmic shear survey will be able to constrain the absolute neutrino mass scale.
A. Refregier +33 more
core +1 more source
Large-Scale Cosmic Shear Measurements
submitted to ApJ ...
Kaiser, Nick +2 more
openaire +2 more sources
Comparing cosmic shear nulling methods for Stage-IV surveys
We present an analysis comparing nulling strategies for reducing the impact of baryon feedback on cosmic shear measurements. We consider three different approaches which aim to `null' the high-$k$ modes using transformations applied to the data vector ...
Naomi Clare Robertson, Alex Hall
doaj +1 more source
Constraints on higher-dimensional gravity from the cosmic shear three-point correlation function
With the developments of large galaxy surveys or cosmic shear surveys it is now possible to map the dark matter distribution at truly cosmological scales.
Bernardeau, Francis
core +1 more source
Diagnosing multiplicative error by lensing magnification of type Ia supernovae
Weak lensing causes spatially coherent fluctuations in flux of type Ia supernovae (SNe Ia). This lensing magnification allows for weak lensing measurement independent of cosmic shear.
Zhang, Pengjie
core +1 more source
We present a comprehensive forecast for cosmological constraints using the joint observation of the cosmic shear signal from the Chinese Space Station Survey Telescope (CSST) and the clustering signal from the next-generation gravitational wave (GW ...
Pengfei Su +6 more
doaj +1 more source
Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
Forthcoming experiments will enable us to determine tomographic shear spectra at a high precision level. Most predictions about them have until now been biased on algorithms yielding the expected linear and non-linear spectrum of density fluctuations ...
Amara +41 more
core +1 more source

