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From the 2 of 77 papers with an AI index.

most citedDESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

68 citations

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17 papers · 1 filter

astro-ph.CO2026

Quintom Model Perturbations

L. W. K. Goh, A. N. Taylor

We build upon the work of Goh and Taylor 2025, in which we proposed a two scalar field quintom framework capable of naturally realising a phantom-to-quintessence transition in the…

astro-ph.CO20261 cited

Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure

Chiara De Leo, Guadalupe Cañas-Herrera, Anna Balaudo +3

We investigate the synergy between large-scale structure (LSS) observations and gravitational wave (GW) events for testing modified gravity. In particular, we forecast the LSS $\ti…

astro-ph.CO2026

Euclid. Populating a dark universe with galaxies using SciPIC

Euclid Collaboration, E. J. Gonzalez, J. Carretero +305

High-fidelity galaxy mocks are crucial for validating analysis pipelines and for cosmological inference. In this context, the Science Pipeline at PIC (SciPIC) is a pipeline specifi…

astro-ph.CO20262 cited

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

Unveiling the dark Universe with HI and EMBER-2

Mauro Bernardini, Robert Feldmann, Daniel Anglés-Alcázar +2

Next-generation radio telescopes will provide unprecedented data volumes of the neutral hydrogen (HI) distribution across cosmic time. The spatial and kinematic distribution of HI…

astro-ph.CO2026

Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters

Samuel Brieden, Florian Beutler, Marcos Pellejero-Ibañez

We present a parameter-free variant of the halo model that significantly improves the precision of matter clustering predictions, particularly in the challenging 1-halo to 2-halo t…