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19962008
most citedA high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets

80 citations · 319 across the 10 of their papers we have counts for

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astro-ph20084 cited

Detecting the B-mode Polarisation of the CMB with Clover

C. E. North, B. R. Johnson, P. A. R. Ade +41

We describe the objectives, design and predicted performance of Clover, which is a ground-based experiment to measure the faint ``B-mode'' polarisation pattern in the cosmic microw…

astro-ph200880 cited

A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets

J. D. McEwen, M. P. Hobson, A. N. Lasenby +1

We repeat the directional spherical real Morlet wavelet analysis, used to detect non-Gaussianity in the Wilkinson Microwave Anisotropy Probe (WMAP) 1-year and 3-year data (McEwen e…

astro-ph200763 cited

A low CMB variance in the WMAP data

C. Monteserin, R. B. Barreiro, P. Vielva +3

We have estimated the CMB variance from the three-year WMAP data, finding a value which is significantly lower than the one expected from Gaussian simulations using the WMAP best-f…

astro-ph200767 cited

Cosmological applications of a wavelet analysis on the sphere

J. D. McEwen, P. Vielva, Y. Wiaux +6

The cosmic microwave background (CMB) is a relic radiation of the Big Bang and as such it contains a wealth of cosmological information. Statistical analyses of the CMB, in conjunc…

astro-ph200745 cited

Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures

J. D. McEwen, Y. Wiaux, M. P. Hobson +2

Using local morphological measures on the sphere defined through a steerable wavelet analysis, we examine the three-year WMAP and the NVSS data for correlation induced by the integ…

astro-ph200736 cited

Constraints on spinning dust towards Galactic targets with the VSA: a tentative detection of excess microwave emission towards 3C396

Anna Scaife, David A. Green, Richard A. Battye +18

We present results from observations made at 33 GHz with the Very Small Array (VSA) telescope towards potential candidates in the Galactic plane for spinning dust emission. In the…