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From the 1 of 8 linked papers with an AI index.

collaborators

8 papers

astro-ph.CO2026

On combining estimated and analytic covariance matrices

Alan Heavens, Lorne Whiteway, Elena Sellentin

The paper derives an accurate multivariate Student‑t approximation for likelihoods that combine covariance matrices estimated from simulations with additional Gaussian error contri…

astro-ph.CO2026

Cluster gravitational redshifts: uncertainties and survey requirements

Eleni Tsaprazi, Giorgio F. Lesci, Federico Marulli +2

We investigate the impact of observational and theoretical uncertainties in cluster gravitational redshifts as a probe of modified gravity using an end-to-end forecasting pipeline.…

astro-ph.CO2026

Dark Energy Survey Year 3 results: optimized CDM simulation-based inference with weak lensing map-level hybrid statistics

J. Williamson, T. L. Makinen, N. Porqueres +85

We present cosmological constraints from the Dark Energy Survey Year 3 (DES Y3) weak lensing data using hierarchical hybrid statistics within a Bayesian simulation-based inference…

astro-ph.CO2026

KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions

George T. Kyriacou, Arrykrishna Mootoovaloo, Alan F. Heavens +3

Tomographic redshift distributions from photometric data are crucial ingredients in cosmic shear analysis, since they are required for the theoretical calculation of the signal bas…

astro-ph.CO2026

Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters

Euclid Collaboration, E. Tsaprazi, A. Fumagalli +274

The \textit{Euclid} satellite will deliver a catalogue of optically-selected galaxy clusters spanning from around deg in Data Release (DR) 1 to around deg

astro-ph.CO2026

Almanac: HMC sampling with bounded velocity

Javier Silva Lafaurie, Lorne Whiteway, Elena Sellentin +4

In Hamiltonian Monte Carlo sampling, the shape of the potential and the choice of the momentum distribution jointly give rise to the Hamiltonian dynamics of the sampler. An efficie…