Controlling intrinsic alignments in weak lensing statistics: The nulling and boosting techniques

Abstract

The intrinsic alignment of galaxies constitutes the major astrophysical source of systematic errors in surveys of weak gravitational lensing by the large-scale structure. We discuss the principles, summarise the implementation, and highlight the performance of two model-independent methods that control intrinsic alignment signals in weak lensing data: the nulling technique which eliminates intrinsic alignments to ensure unbiased constraints on cosmology, and the boosting technique which extracts intrinsic alignments and hence allows one to further study this contribution. Making only use of the characteristic dependence on redshift of the signals, both approaches are robust, but reduce the statistical power due to the similar redshift scaling of intrinsic alignment and lensing signals.

10 pages, 6 figures; to appear in the proceedings of Astronomical Data Analysis 6, Monastir, Tunisia, 3-7 May 2010

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• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Intrinsic and extrinsic correlations of galaxy shapes and sizes in weak lensing data