A Prediction for DESI Full-Shape: Increasing Tomographic m(z) Trend
astro-ph.CO
Submitted: 2026-08-20
Updated: 2026-08-31
Terminology
Sources
- In the Realm of the Hubble tension $-$ a Review of Solutions
- Hubble Tension: The Evidence of New Physics
- The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Running Hubble Tension and a H0 Diagnostic
- $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
- Planck 2018 results. VI. Cosmological parameters
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Measurements of the Hubble Constant: Tensions in Perspective
- The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
- Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
- CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
- Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
- TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography
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