The impact of high spatial frequency atmospheric distortions on weak lensing measurements
High precision cosmology with weak gravitational lensing requires a precise measure of the Point Spread Function across the imaging data where the accuracy to which high spatial frequency variation can be modelled is limited by the stellar number density across the field. We analyse dense stellar fi...
Egile Nagusiak: | Heymans, C, Rowe, B, Hoekstra, H, Miller, L, Erben, T, Kitching, T, Waerbeke, L |
---|---|
Formatua: | Journal article |
Hizkuntza: | English |
Argitaratua: |
2011
|
Antzeko izenburuak
-
The impact of high spatial frequency atmospheric distortions on weak-lensing measurements
nork: Heymans, C, et al.
Argitaratua: (2012) -
Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -II.
Application to Simulations
nork: Kitching, T, et al.
Argitaratua: (2008) -
CFHTLenS: Testing the Laws of Gravity with Tomographic Weak Lensing and
Redshift Space Distortions
nork: Simpson, F, et al.
Argitaratua: (2012) -
Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I.
Methodology and a Fast Fitting Algorithm
nork: Miller, L, et al.
Argitaratua: (2007) -
Bayesian Galaxy Shape Measurement for Weak Lensing Surveys - III.
Application to the Canada-France-Hawaii Telescope Lensing Survey
nork: Miller, L, et al.
Argitaratua: (2012)