Parameterizations of the Hubble Constant from the Binned Type Ia Supernova Master Sample: Logarithmic versus Power-law Forms
astro-ph.CO
Submitted: 2026-02-28
Updated: 2026-09-19
Comments: 28 pages, 4 figures, Accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
- A gravitational-wave standard siren measurement of the Hubble constant
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817
- Constraints on the cosmic expansion history from GWTC-3
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Planck 2015 results. XIII. Cosmological parameters
- Planck 2018 results. VI. Cosmological parameters
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
- Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
- The Cosmic Triangle: Revealing the State of the Universe
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
- TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
- H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
- Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
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