Tracing the Evolution of m(z) over the Last 10 Billion Years with Non-parametric Methods

arXiv:2603.25851 · astro-ph.CO, gr-qc · Submitted 2026-03-26 · Read on arXiv

astro-ph.CO, gr-qc

Submitted: 2026-03-26

Updated: 2026-09-22

Terminology

• Calibration — 41× in this paper · explained in 7 episodes
• Gaussian Process Regression — 4× in this paper
• Clustering — 3× in this paper · explained in 2 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Hubble Tension — 2× in this paper · explained in 9 episodes
• Robustness — 2× in this paper · explained in 5 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Planck and the South Pole Telescope — 1× in this paper
• Weak Lensing — 1× in this paper · explained in 2 episodes

Sources

• Cosmology with Galaxy Clusters
• Cosmological Parameters from Observations of Galaxy Clusters
• The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
• Formation of Galaxy Clusters
• Non-Parametric Analysis for the Dark Matter Density Evolution
• A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
• Probing the dark matter density evolution law with large scale structures
• An estimate of the dark matter density from galaxy clusters and supernovae data
• Cosmology with galaxy clusters using machine learning. Application to eROSITA Data
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Status of the $S_8$ Tension: A 2026 Review of Probe Discrepancies
• Cluster-galaxy weak lensing
• Optical selection bias and projection effects in stacked galaxy cluster weak lensing
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• Turbulent pressure support and hydrostatic mass-bias in the intracluster medium
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• Can vacuum decay in our Universe?
• Renormalization-Group Improved Effective Lagrangian for Interacting Theories in Curved Spacetime
• The Effective Action in Gauged Supergravity on Hyperbolic Background and Induced Cosmological Constant

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