activity
20052008
most citedBayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm

250 citations · 880 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph2008133 cited

Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -II. Application to Simulations

T. D. Kitching, L. Miller, C. E. Heymans +2

We extend the Bayesian model fitting shape measurement method presented in Miller et al. (2007) and use the method to estimate the shear from the Shear TEsting Programme simulation…

astro-ph2008120 cited

Handbook for the GREAT08 Challenge: An image analysis competition for cosmological lensing

Sarah Bridle, John Shawe-Taylor, Adam Amara +35

The GRavitational lEnsing Accuracy Testing 2008 (GREAT08) Challenge focuses on a problem that is of crucial importance for future observations in cosmology. The shapes of distant g…

astro-ph200893 cited

Finding Evidence for Massive Neutrinos using 3D Weak Lensing

T. D. Kitching, A. F. Heavens, L. Verde +2

In this paper we investigate the potential of 3D cosmic shear to constrain massive neutrino parameters. We find that if the total mass is substantial (near the upper limits from LS…

astro-ph2007250 cited

Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm

L. Miller, T. D. Kitching, C. Heymans +2

The principles of measuring the shapes of galaxies by a model-fitting approach are discussed in the context of shape-measurement for surveys of weak gravitational lensing. It is ar…

astro-ph200678 cited

Cosmological constraints from COMBO-17 using 3D weak lensing

T. D. Kitching, A. F. Heavens, A. N. Taylor +5

We present the first application of the 3D cosmic shear method developed in Heavens et al. (2006) and the geometric shear-ratio analysis developed in Taylor et al. (2006), to the C…

astro-ph200685 cited

Measuring dark energy properties with 3D cosmic shear

A. F. Heavens, T. D. Kitching, A. N. Taylor

We present parameter estimation forecasts for present and future 3D cosmic shear surveys. We demonstrate that, in conjunction with results from cosmic microwave background (CMB) ex…