#large-scale structure

topiclarge-scale structure

33 papers · 1 filter

astro-ph.CO2026

The Dark Energy Camera All Data Everywhere cosmic shear project V: Constraints on cosmology and astrophysics from 270 million galaxies across 13,000 deg of the sky

D. Anbajagane, C. Chang, A. Drlica-Wagner +78

The paper presents cosmological and astrophysical constraints derived from cosmic shear measurements of 270 million galaxies covering 13,000 deg², combining data from the DECADE pr…

astro-ph.CO2026

A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics

2pt Collaboration, Elisabeth Krause, Yosuke Kobayashi +23

The paper presents the first results of the "Beyond-2pt" community data challenge, where participants used various beyond‑two‑point galaxy clustering methods on high‑precision mock…

astro-ph.CO2026

Dynamic Zoom Simulations of structure formation beyond standard cosmology

Riccardo Zangarelli, Marco Baldi, Federico Marinacci +1

The paper introduces a Dynamic Zoom Simulations (DZS) technique that reduces resolution outside an observer’s lightcone to speed up large‑scale cosmological simulations, and valida…

astro-ph.CO2026

Cross-Correlating the Universe: The Gravitational Wave Background and Large-Scale Structure

Federico Semenzato, J. Andrew Casey-Clyde, Chiara M. F. Mingarelli +4

The paper proposes using cross‑correlations between gravitational‑wave background anisotropy maps and galaxy surveys to detect the imprint of unresolved supermassive black‑hole bin…

astro-ph.CO2026

Mitigating galaxy systematics with gravitational wave clustering

Caterina Scarpel, Nicola Bellomo, Sarah Libanore +2

The paper demonstrates that clustering of gravitational‑wave events can be used as a complementary tracer to galaxies, reducing systematic errors and improving constraints on local…

astro-ph.CO2026

Constraints on Ultra-Light Axions from the DESI DR1 Full Shape, Planck and ACT

Francesco Verdiani, Emanuele Castorina, Ennio Salvioni +2

The paper derives new limits on ultra-light axions as a small part of dark matter using galaxy clustering data from DESI DR1 together with CMB measurements from Planck and ACT.