activity
20062020
most citedCosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data

156 citations · 670 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.CO2020★ 8 cited

Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data

Lucas Porth, Robert E. Smith, Patrick Simon +2

We explore an alternative method to the usual shear correlation function approach for the estimation of aperture mass statistics in weak lensing survey data. Our approach builds on…

astro-ph.CO2016★ 156 cited

Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data

T. Kacprzak, D. Kirk, O. Friedrich +81

Shear peak statistics has gained a lot of attention recently as a practical alternative to the two point statistics for constraining cosmological parameters. We perform a shear pea…

astro-ph.CO2015★ 5 cited

What is the optimal way to measure the galaxy power spectrum?

Robert E. Smith, Laura Marian

Measurements of the galaxy power spectrum contain a wealth of information about the Universe. Its optimal extraction is vital if we are to truly understand the micro-physical natur…

astro-ph.CO2015★ 16 cited

Towards optimal estimation of the galaxy power spectrum

Robert E. Smith, Laura Marian

The galaxy power spectrum encodes a wealth of information about cosmology and the matter fluctuations. Its unbiased and optimal estimation is therefore of great importance. In this…

astro-ph.CO2014

An exploration of galaxy-galaxy lensing and galaxy clustering in the Millennium-XXL simulation

Laura Marian, Robert E. Smith, Raul E. Angulo

The combination of galaxy-galaxy lensing and galaxy clustering data has the potential to simultaneously constrain both the cosmological and galaxy formation models. In this paper w…

astro-ph.CO2014★ 6 cited

Toward optimal cluster power spectrum analysis

Robert E. Smith, Laura Marian

The power spectrum of galaxy clusters is an important probe of the cosmological model. In this paper we determine the optimal weighting scheme for maximizing the signal-to-noise ra…