Discrepancies between CFHTLenS cosmic shear & Planck: new physics or systematic effects?
Thomas D. Kitching, Licia Verde, Alan F. Heavens, Raul Jimenez

TL;DR
This study investigates the discrepancy between cosmic shear measurements from CFHTLenS and Planck CMB data, exploring potential systematic effects and new physics such as neutrinos or modified gravity, using a non-parametric baryon feedback model and 3D cosmic shear analysis.
Contribution
It applies a flexible non-parametric baryonic feedback model and 3D cosmic shear methodology to CFHTLenS data, assuming Planck parameters, to assess systematics and constraints on neutrino masses.
Findings
No evidence for baryonic feedback effects.
Detected a bias in photometric redshifts.
Upper limit on neutrino mass: < 0.28 eV.
Abstract
There is currently a discrepancy in the measured value of the amplitude of matter clustering, parameterised using , inferred from galaxy weak lensing, and cosmic microwave background data, which could be an indication of new physics, such as massive neutrinos or a modification to the gravity law, or baryon feedback. In this paper we make the assumption that the cosmological parameters are well determined by Planck, and use weak lensing data to investigate the implications for baryon feedback and massive neutrinos, as well as possible contributions from intrinsic alignments and biases in photometric redshifts. We apply a non-parametric approach to model the baryonic feedback on the dark matter clustering, which is flexible enough to reproduce the OWLS and Illustris simulation results. The statistic we use, 3D cosmic shear, is a method that extracts cosmological information from…
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