most citedQuasi-automatic software support for Gaia ground based optical tracking

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astro-ph.CO2026

Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review

Rogério Monteiro-Oliveira

Merging galaxy clusters represent one of the most powerful macroscopic laboratories in the Universe for searching for new physics within the dark sector. High-velocity cosmic colli…

astro-ph.CO2026

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime

Fernanda Oliveira, Miguel A. Sabogal, Felipe Avila +2

We investigate recent reports of a suppression in the growth rate of cosmic structures inferred from analyses of the dataset. To address this issue, we explore the hyp…

astro-ph.CO2026

Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking

Xiaoyun Shao, Facundo Toscano, Diego Garcia Lambas +5

The Cosmic Microwave Background (CMB) reaches homogeneity at relatively modest angular scales compared to the expectation of the standard CDM model revealing an important chall…

astro-ph.CO20265 cited

A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations

Felipe Bruno Medeiros dos Santos, Jonathan Morais, Supriya Pan +2

Baryon acoustic oscillation (BAO) data from the Dark Energy Spectroscopic Instrument (DESI) appear to indicate the first evidence for dynamical dark energy (DDE), with a present-da…

astro-ph.CO2026

Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB

Camilo Crisman, Miguel Quartin, João Rebouças

Type Ia supernova (SN) magnitudes present correlations due to the fact that their peculiar velocities are sourced by the large-scale structure of the Universe. This effect can be u…

astro-ph.CO2026

Euclid preparation. CIV. Impact of galaxy intrinsic alignment modelling choices on Euclid 3x2pt cosmology

Euclid Collaboration, D. Navarro-Gironés, I. Tutusaus +274

The Euclid galaxy survey will provide unprecedented constraints on cosmology, but achieving unbiased results will require an optimal characterisation and mitigation of systematic e…