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19962022
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 29.9k across the 266 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 16 cited

Sunyaev-Zel'dovich Cluster Survey Simulations for Planck

Joern Geisbuesch, Ruediger Kneissl, Michael Hobson

We examine the ability of the future Planck mission to provide a catalogue of galaxy clusters observed via their SZ distortion in the cosmic microwave background. For this purpose…

astro-ph2004★ 60 cited

Simulation of non-Gaussian CMB maps

Graca Rocha, M. P. Hobson, Sarah Smith +2

A simple method is presented for the rapid simulation of statistically-isotropic non-Gaussian maps of CMB temperature fluctuations with a given power spectrum and analytically-calc…

astro-ph2004★ 4 cited

Cosmological parameter estimation with large scale structure and supernovae data

Carolina Odman, Mike Hobson, Anthony Lasenby +1

Most cosmological parameter estimations are based on the same set of observations and are therefore not independent. Here, we test the consistency of parameter estimations using a…

astro-ph2004★ 95 cited

Cosmological parameter estimation using Very Small Array data out to l=1500

Rafael Rebolo, Richard A. Battye, Pedro Carreira +29

We estimate cosmological parameters using data obtained by the Very Small Array (VSA) in its extended configuration, in conjunction with a variety of other CMB data and external pr…

astro-ph2004★ 207 cited

High sensitivity measurements of the CMB power spectrum with the extended Very Small Array

Clive Dickinson, Richard A. Battye, Kieran Cleary +29

We present deep Ka-band ( GHz) observations of the CMB made with the extended Very Small Array (VSA). This configuration produces a naturally weighted synthesized FWHM…

astro-ph2004★ 19 cited

Estimating the bispectrum of the Very Small Array data

Sarah Smith, Graca Rocha, Anthony Challinor +30

We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in December 2002, and compare our results to those obtaine…