Volume 479, Number 3, March I 2008
|Page(s)||655 - 667|
|Section||Cosmology (including clusters of galaxies)|
|Published online||02 January 2008|
First detection of galaxy-galaxy-galaxy lensing in RCS*
A new tool for studying the matter environment of galaxy pairs
The Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, School of Physics, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK e-mail: email@example.com
2 Argelander-Institut für Astronomie (Founded by merging of the Institut für Astrophysik und Extraterrestrische Forschung, the Sternwarte, and the Radioastronomisches Institut der Universität Bonn. ) , Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
3 Department of Physics and Astronomy, University of Victoria, Victoria, BC, V8P 5C2, Canada
4 Department of Astronomy & Astrophysics, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA
5 Department of Astronomy & Astrophysics, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
6 Institute of Astrophysics & Astronomy, Academia Sinica, PO Box 23-141, Taipei 106, R.O.C. Taiwan
7 Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
Accepted: 17 December 2007
Context.The weak gravitational lensing effect, small coherent distortions of galaxy images by means of a gravitational tidal field, can be used to study the relation between the matter and galaxy distribution.
Aims.In this context, weak lensing has so far only been used for considering a second-order correlation function that relates the matter density and galaxy number density as a function of separation. We implement two new, third-order correlation functions that have recently been suggested in the literature, and apply them to the Red-Sequence Cluster Survey. As a step towards exploiting these new correlators in the future, we demonstrate that it is possible, even with already existing data, to make significant measurements of third-order lensing correlations.
Methods.We develop an optimised computer code for the correlation functions. To test its reliability a set of tests involving mock shear catalogues are performed. The correlation functions are transformed to aperture statistics, which allow easy tests for remaining systematics in the data. In order to further verify the robustness of our measurement, the signal is shown to vanish when randomising the source ellipticities. Finally, the lensing signal is compared to crude predictions based on the halo-model.
Results.On angular scales between ~ and ~ a significant third-order correlation between two lens positions and one source ellipticity is found. We discuss this correlation function as a novel tool to study the average matter environment of pairs of galaxies. Correlating two source ellipticities and one lens position yields a less significant but nevertheless detectable signal on a scale of ~. Both signals lie roughly within the range expected by theory which supports their cosmological origin.
Key words: galaxies: halos / cosmology: large-scale structure of Universe / cosmology: dark matter / cosmology: observations
© ESO, 2008
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