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...

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Détails bibliographiques
Auteurs principaux: Miller, L, Kitching, T, Heymans, C, Heavens, A, Waerbeke, L
Format: Journal article
Langue:English
Publié: 2007