Shi, X., Schneider, P. and Joachimi, B. (2011). Relations between three-point configuration space shear and convergence statistics. Astron. Astrophys., 533. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

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Abstract

With the growing interest in and ability of using weak lensing studies to probe the non-Gaussian properties of the matter density field, there is an increasing need for the study of suitable statistical measures, e.g. shear three-point statistics. In this paper we establish the relations between the three-point configuration space shear and convergence statistics, which are an important missing link between different weak lensing three-point statistics and provide an alternative way of relating observation and theory. The method we use also allows us to derive the relations between other two- and three-point correlation functions. We show the consistency of the relations obtained with already established results and demonstrate how they can be evaluated numerically. As a direct application, we use these relations to formulate the condition for E/B-mode decomposition of lensing three-point statistics, which is the basis for constructing new three-point statistics which allow for exact E/B-mode separation. Our work applies also to other two-dimensional polarization fields such as that of the cosmic microwave background.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Shi, X.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Schneider, P.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Joachimi, B.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-489508
DOI: 10.1051/0004-6361/201117236
Journal or Publication Title: Astron. Astrophys.
Volume: 533
Date: 2011
Publisher: EDP SCIENCES S A
Place of Publication: LES ULIS CEDEX A
ISSN: 1432-0746
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
COSMIC SHEAR; DARK-MATTER; B-MODE; SKEWNESSMultiple languages
Astronomy & AstrophysicsMultiple languages
URI: http://kups.ub.uni-koeln.de/id/eprint/48950

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