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20112026
most citedNon-Gaussianity in Large Scale Structure and Minkowski Functionals

35 citations · 155 across the 11 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2016★ 33 cited

Effect of lensing non-Gaussianity on the CMB power spectra

Antony Lewis, Geraint Pratten

Observed CMB anisotropies are lensed, and the lensed power spectra can be calculated accurately assuming the lensing deflections are Gaussian. However, the lensing deflections are…

astro-ph.CO2016★ 18 cited

3D Weak Lensing: Modified Theories of Gravity

Geraint Pratten, Dipak Munshi, Patrick Valageas +1

Weak lensing (WL) promises to be a particularly sensitive probe of both the growth of large scale structure (LSS) as well as the fundamental relation between matter density perturb…

astro-ph.CO2015★ 14 cited

Galaxy Clustering in 3D and Modified Gravity Theories

Dipak Munshi, Geraint Pratten, Patrick Valageas +2

We study Modified Gravity (MG) theories by modelling the redshifted matter power spectrum in a spherical Fourier-Bessel (sFB) basis. We use a fully non-linear description of the re…

astro-ph.CO2014★ 6 cited

Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D

Geraint Pratten, Dipak Munshi

The thermal Sunyaev-Zel'dovich (tSZ) effect measures the line-of-sight projection of the thermal pressure of free electrons and lacks any redshift information. By cross correlating…

astro-ph.CO2013★ 22 cited

Effects of Linear Redshift Space Distortions and Perturbation Theory on BAOs: A 3D Spherical Analysis

Geraint Pratten, Dipak Munshi

The Baryon Acoustic Oscillations (BAO) are features in the matter power spectrum on scales of order 100-150 h^{-1} Mpc that promise to be a powerful tool to constrain and test cosm…

astro-ph.CO2011★ 35 cited

Non-Gaussianity in Large Scale Structure and Minkowski Functionals

Geraint Pratten, Dipak Munshi

Minkowski Functionals (MFs) are topological statistics that have become one of many standard tools used for investigating the statistical properties of cosmological random fields.…