activity
20172026
most citedThe third data release of the Kilo-Degree Survey and associated data products

219 citations · 563 across the 10 of their papers we have counts for

collaborators
Showing 2025Show all

5 papers · 1 filter

astro-ph.CO2025

A roadmap to cosmological parameter analysis with third-order shear statistics IV. Analytic cross-covariance between second- and third-order aperture masses

Niek Wielders, Laila Linke, Pierre A. Burger +3

Weak gravitational lensing is a powerful probe of cosmology, with second-order shear statistics commonly used to constrain parameters such as the matter density and…

astro-ph.CO2025★ 1 cited

Towards an application of fourth-order shear statistics II: Efficient estimation of fourth-order shear correlation functions and an application to the DES Y3 data

Lucas Porth, Elena Silvestre-Rosello, Peter Schneider +1

Higher-order lensing statistics contain a wealth of cosmological information that is not captured by second-order statistics. Stage-III lensing surveys have sufficient statistical…

astro-ph.CO2025

Towards an application of fourth-order shear statistics I. The information content of

Elena Silvestre-Rosello, Lucas Porth, Peter Schneider +4

Higher-order shear statistics contain part of the non-Gaussian information of the projected matter field and therefore can provide additional constraints on the cosmological parame…

astro-ph.GA2025★ 44 cited

The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields

Angus H. Wright, Konrad Kuijken, Hendrik Hildebrandt +51

We present the final data release of the Kilo-Degree Survey (KiDS-DR5), a public European Southern Observatory (ESO) wide-field imaging survey optimised for weak gravitational lens…

astro-ph.CO2025★ 119 cited

KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey

Angus H. Wright, Benjamin Stölzner, Marika Asgari +35

We present cosmic shear constraints from the completed Kilo-Degree Survey (KiDS), where the cosmological parameter , is…