activity
20162025
most citedKiDS-1000 Cosmology: constraints beyond flat CDM

134 citations · 502 across the 12 of their papers we have counts for

collaborators

12 papers

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.CO2021★ 43 cited

On the road to percent accuracy V: the non-linear power spectrum beyond CDM with massive neutrinos and baryonic feedback

Benjamin Bose, Bill S. Wright, Matteo Cataneo +7

In the context of forthcoming galaxy surveys, to ensure unbiased constraints on cosmology and gravity when using non-linear structure information, percent-level accuracy is require…

astro-ph.CO2020★ 81 cited

Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1

Joachim Harnois-Déraps, Nicolas Martinet, Tiago Castro +5

We constrain cosmological parameters from a joint cosmic shear analysis of peak-counts and the two-point shear correlation functions, as measured from the Dark Energy Survey (DES-Y…

astro-ph.CO2020★ 134 cited

KiDS-1000 Cosmology: constraints beyond flat CDM

Tilman Tröster, Marika Asgari, Chris Blake +26

We present constraints on extensions to the flat CDM cosmological model by varying the spatial curvature , the sum of the neutrino masses , the dark energy equati…

astro-ph.CO2020★ 25 cited

Intergalactic filaments spin

Qianli Xia, Mark C. Neyrinck, Yan-Chuan Cai +1

Matter in the Universe is arranged in a cosmic web, with a filament of matter typically connecting each neighbouring galaxy pair, separated by tens of millions of light-years. A qu…

astro-ph.CO2020★ 75 cited

On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond CDM

Benjamin Bose, Matteo Cataneo, Tilman Tröster +3

To effectively exploit large-scale structure surveys, we depend on accurate and reliable predictions of non-linear cosmological structure formation. Tools for efficient and compreh…