works on

From the 1 of 21 linked papers with an AI index.

activity
20242026
collaborators

21 papers

astro-ph.CO2026

Probabilistic redshift estimation of unresolved galaxies from multi-band background light maps

Shun-Sheng Li, Hendrik Hildebrandt, Ludovic Van Waerbeke

The paper introduces a method that uses conditional normalising flows trained on realistic simulations to estimate redshift distributions of unresolved galaxies directly from multi…

astro-ph.CO2026

KiDS-Legacy: The consistency test of the large-scale structure with Bernardeau-Nishimichi-Taruya transform

Shiming Gu, Ziang Yan, Ludovic van Waerbeke +10

We perform the first -cut cosmic shear analysis of the KiDS-Legacy survey. This method uses the Bernardeau-Nishimichi-Taruya (BNT) transform to construct weak-lensing kernels th…

astro-ph.CO2026

KiDS-Legacy: Joint analysis of second- and third-order cosmic shear

L. Linke, L. Porth, P. Burger +21

Weak lensing by large-scale structure is a powerful cosmological probe. While most analyses rely on second-order correlations, these are primarily sensitive to the parameter combin…

astro-ph.CO2026

KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature

Robert Reischke, Benjamin Stölzner, Benjamin Joachimi +25

We constrained minimally extended cosmological models with the cosmic shear analysis of the final data release from the Kilo-Degree Survey (KiDS-Legacy) in combination with externa…

astro-ph.CO2026

KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies

Benjamin Stölzner, Robert Reischke, Matteo Grasso +25

We present constraints on modified gravity from a cosmic shear analysis of the final data release of the Kilo-Degree Survey (KiDS-Legacy) in combination with DESI measurements of b…

astro-ph.CO2026

pop-cosmos: Forward modeling KiDS-1000 redshift distributions using realistic galaxy populations

Boris Leistedt, Hiranya V. Peiris, Anik Halder +13

The accuracy of the cosmological constraints from Stage~IV galaxy surveys will be limited by how well the galaxy redshift distributions can be inferred. We have addressed this chal…