Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm
The principles of measuring the shapes of galaxies by a model-fitting approach are discussed in the context of shape-measurement for surveys of weak gravitational lensing. It is argued that such an approach should be optimal, allowing measurement with maximal signal-to-noise, coupled with estimation...
Κύριοι συγγραφείς: | Miller, L, Kitching, T, Heymans, C, Heavens, A, Waerbeke, L |
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Μορφή: | Journal article |
Γλώσσα: | English |
Έκδοση: |
2007
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Παρόμοια τεκμήρια
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The impact of high spatial frequency atmospheric distortions on weak-lensing measurements
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