201. An optimal filter for the detection of galaxy clusters through weak lensing
- Author
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Lauro Moscardini, Matthias Bartelmann, Massimo Meneghetti, Klaus Dolag, Matteo Maturi, MATURI M., MENEGHETTI M., BARTELMANN M., DOLAG K., and MOSCARDINI L.
- Subjects
Physics ,Astrophysics (astro-ph) ,Shot noise ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Filter (signal processing) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Galaxy ,Computational physics ,Noise ,Space and Planetary Science ,Halo ,Galaxy cluster ,Weak gravitational lensing ,Linear filter - Abstract
We construct a linear filter optimised for detecting dark-matter halos in weak-lensing data. The filter assumes a mean radial profile of the halo shear pattern and modifies that shape by the noise power spectrum. Aiming at separating dark-matter halos from spurious peaks caused by large-scale structure lensing, we model the noise as being composed of weak lensing by large-scale structures and Poisson noise from random galaxy positions and intrinsic ellipticities. Optimal filtering against the noise requires the optimal filter scale to be smaller than typical halo sizes. Although a perfect separation of halos from spurious large-scale structure peaks is strictly impossible, we use numerical simulations to demonstrate that our filter produces substantially more sensitive, reliable and stable results than the conventionally used aperture-mass statistic., Comment: 9 pages, 6 figures, A&A submitted
- Published
- 2004
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