activity
20162022
most citedTowards emulating cosmic shear data: Revisiting the calibration of the shear measurements for the Kilo-Degree Survey

95 citations · 698 across the 18 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

astro-ph.CO2018★ 95 cited

Towards emulating cosmic shear data: Revisiting the calibration of the shear measurements for the Kilo-Degree Survey

Arun Kannawadi, Henk Hoekstra, Lance Miller +9

Exploiting the full statistical power of future cosmic shear surveys will necessitate improvements to the accuracy with which the gravitational lensing signal is measured. We prese…

astro-ph.CO2018★ 25 cited

Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurements

Mohammadjavad Vakili, Maciej Bilicki, Henk Hoekstra +5

We use the overlap between multiband photometry of the Kilo-Degree Survey (KiDS) and spectroscopic data based on the Sloan Digital Sky Survey (SDSS) and Galaxy And Mass Assembly (G…

astro-ph.CO2018★ 78 cited

Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum

Manuel Colavincenzo, Emiliano Sefusatti, Pierluigi Monaco +19

We compare the measurements of the bispectrum and the estimate of its covariance obtained from a set of different methods for the efficient generation of approximate dark matter ha…

astro-ph.CO2018★ 86 cited

Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles

Linda Blot, Martin Crocce, Emiliano Sefusatti +19

We study the accuracy of several approximate methods for gravitational dynamics in terms of halo power spectrum multipoles and their estimated covariance matrix. We propagate the d…

astro-ph.CO2018★ 84 cited

Comparing approximate methods for mock catalogues and covariance matrices I: correlation function

Martha Lippich, Ariel G. Sánchez, Manuel Colavincenzo +19

This paper is the first in a set that analyses the covariance matrices of clustering statistics obtained from several approximate methods for gravitational structure formation. We…