The case for non-Gaussianity on cluster scales
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/353/2/681/3876863/353-2-681.pdf
Reference47 articles.
1. Power spectrum normalization and the non-Gaussian halo model
2. Cosmological perturbations and the reionization epoch
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4. The Effects of Non‐Gaussian Initial Conditions on the Structure and Substructure of Cold Dark Matter Halos
5. The Cluster Mass Function from Early Sloan Digital Sky Survey Data: Cosmological Implications
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1. Constraints on non-Gaussianity from Sunyaev-Zeldovich cluster surveys;Physical Review D;2012-12-18
2. Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion;Journal of Cosmology and Astroparticle Physics;2012-10-12
3. Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks;Monthly Notices of the Royal Astronomical Society;2011-08-31
4. The effect of primordial non-Gaussianity on the skeleton of cosmic shear maps;Monthly Notices of the Royal Astronomical Society;2011-08-11
5. SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS OF STRONG LENSING GALAXY CLUSTERS: PROBING THE OVERCONCENTRATION PROBLEM;The Astrophysical Journal;2011-08-08
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