Two-rung ladder: H 0 from Tip of the Red Giant Branch and geometric anchors alone
astro-ph.CO, astro-ph.GA
Submitted: 2026-09-24
Updated: 2026-09-24
Comments: 22 pages, 9 figures, 3 tables. Submitted to MNRAS
License: http://creativecommons.org/licenses/by/4.0/
The gist: We infer the Hubble constant H 0 from the 400 Extragalactic Distance Database hosts with a tip of the red giant branch (TRGB) distance, calibrated on the geometric anchors of the Large Magellanic
Terminology
Abstract
We infer the Hubble constant H 0 from the 400 Extragalactic Distance Database hosts with a tip of the red giant branch (TRGB) distance, calibrated on the geometric anchors of the Large Magellanic Cloud and NGC 4258. We forward-model the tip magnitudes and host redshifts including magnitude-limited selection, sky exposure, and density-dependent galaxy bias, conditioning on each of the 80 Manticore-Local realisations of the local density and peculiar-velocity fields in turn. As most hosts lie at cz CMB 1000 km/s, where peculiar velocities are important, the inference is limited by the variance of these fields rather than by the TRGB calibration. For a fixed realisation, the redshift likelihood and density smoothing each move H 0 by less than 1 km/s/Mpc and a velocity monopole by 5.4 plus or minus 3.4 km/s/Mpc, whereas the field-to-field scatter in H 0 is 5.2 km/s/Mpc. Weighting the posteriors from each realisation equally gives H 0 = 68.4 plus or minus 5.9 km/s/Mpc, while weighting each by its Bayesian evidence gives 72.3 plus or minus 2.6 km/s/Mpc. The latter value is set by a single particularly high-evidence realisation, making it sensitive to the finite sampling of the reconstruction posterior. This ladder therefore cannot yet arbitrate the Hubble tension. Extending the TRGB data beyond the present 1000 km/s, together with improved reconstructions of the local Universe, would reduce the field-to-field scatter well below the 5.2 km/s/Mpc we find here.
Sources
- Gathering Galaxy Distances in Abundance with Roman Wide-Area Data
- Surface Brightness Fluctuations
- Illuminating the Local Universe: Large-Scale Structure from ZTF Type Ia Supernovae
- Accounting for sample selection in Bayesian analyses
- The No-U-Turn Sampler: Adaptively Setting Path Lengths in Hamiltonian Monte Carlo
- The Tip of the Red Giant Branch Distance Ladder and the Hubble Constant
- Machine learning assisted Bayesian model comparison: learnt harmonic mean estimator
- Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro
- Learned harmonic mean estimation of the marginal likelihood with normalizing flows
- A reanalysis of the megamaser Hubble constant: from spot catalogues to peculiar velocities
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