Cosmic microwave background temperature cosmography

arXiv:2607.23535 · astro-ph.CO, gr-qc, hep-ph · Submitted 2026-07-26 · Read on arXiv

C. J. A. P. Martins

astro-ph.CO, gr-qc, hep-ph

Submitted: 2026-07-26

Comments: 5 pages, 4 figures, 4 tables; letter published in MNRAS

DOI: 10.1093/mnras/stag1315

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Accuracy — 2× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes

Related papers

• Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
• Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
• Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
• Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation