output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2010 · astro-ph.COShow all

18 papers · 2 filters

astro-ph.CO2010★ 53 cited

Accurate Modeling of Weak Lensing with the sGL Method

Kimmo Kainulainen, Valerio Marra

We revise and extend the stochastic approach to cumulative weak lensing (hereafter the sGL method) first introduced in Ref. [1]. Here we include a realistic halo mass function and…

astro-ph.CO2010★ 15 cited

On the role of shear in cosmological averaging II: large voids, non-empty voids and a network of different voids

Maria Mattsson, Teppo Mattsson

We study the effect of shear on the cosmological backreaction in the context of matching voids and walls together using the exact inhomogeneous Lemaitre-Tolman-Bondi solution. Gene…

astro-ph.CO2010★ 8 cited

The self-interacting curvaton

Kari Enqvist

The evolution of the curvature perturbation is highly non-trivial for curvaton models with self-interactions and is very sensitive to the parameter values. The final perturbation d…

astro-ph.CO2010★ 32 cited

Estimating f_NL and g_NL from Massive High-Redshift Galaxy Clusters

Kari Enqvist, Shaun Hotchkiss, Olli Taanila

There are observations of 15 high-redshift massive galaxy clusters, which have an extremely small probability with a purely Gaussian initial curvature perturbation. Here we revisit…

astro-ph.CO2010★ 183 cited

Short-lived star-forming giant clumps in cosmological simulations of z~2 disks

Shy Genel, Thorsten Naab, Reinhard Genzel +7

Many observed massive star-forming z\approx2 galaxies are large disks that exhibit irregular morphologies, with \sim1kpc, \sim10^(8-10)Msun clumps. We present the largest sample to…

astro-ph.CO2010★ 9 cited

Suzaku observations of X-ray excess emission in the cluster of galaxies A3112

T. Lehto, J. Nevalainen, M. Bonamente +2

We analysed the Suzaku XIS1 data of the A3112 cluster of galaxies in order to examine the X-ray excess emission in this cluster reported earlier with the XMM-Newton and Chandra sat…