Pith. sign in

REVIEW 19 cited by

JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2408.11770 v2 pith:XBI4J4F3 submitted 2024-08-21 astro-ph.CO

JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0

classification astro-ph.CO
keywords jwstsampledifferencescepheidcepheidsfullsamplessneia
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

JWST provides new opportunities to cross-check the HST Cepheid/SNeIa distance ladder, which yields the most precise local measure of H0. We analyze early JWST subsamples (~1/4 of the HST sample) from the SH0ES and CCHP groups, calibrated by a single anchor (N4258). We find HST Cepheid distances agree well (~1 sigma) with all 8 combinations of methods, samples, and telescopes: JWST Cepheids, TRGB, and JAGB by either group, plus HST TRGB and Miras. The comparisons explicitly include the measurement uncertainty of each method in N4258, an oft-neglected but dominant term. Mean differences are ~0.03 mag, far smaller than the 0.18 mag "Hubble tension." Combining all measures produces the strongest constraint yet on the linearity of HST Cepheid distances, 0.994+-0.010, ruling out distance-dependent bias or offset as the source of the tension at ~7 sigma. Yet, measurements of H0 from current JWST subsamples produce large sampling differences whose size and direction we can directly estimate from the full HST set. We show that Delta(H0)~2.5 km/s/Mpc between the CCHP JWST program and the full HST sample is entirely consistent with differences in sample selection. Combining all JWST samples produces a new, distance-limited set of 16 SNeIa at D<25 Mpc and more closely resembles the full sample thanks to "reversion to the mean" of larger samples. Using JWST Cepheids, JAGB, and TRGB, we find 73.4+-2.1, 72.2+-2.2, and 72.1+-2.2 km/s/Mpc, respectively. Explicitly accounting for SNe in common, the combined-sample three-method result from JWST is H0=72.6+-2.0, similar to H0=72.8 expected from HST Cepheids in the same galaxies. The small JWST sample trivially lowers the Hubble tension significance due to small-sample statistics and is not yet competitive with the HST set (42 SNeIa and 4 anchors), which yields 73.2+-0.9. Still, the joint JWST sample provides important crosschecks which the HST data passes.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 19 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions

    astro-ph.CO 2026-05 unverdicted novelty 7.0

    Any unified early and late dark energy scenario with a single tracking scalar field requires a potential with three distinct slopes arranged in a steep-steeper-shallow hierarchy.

  2. $\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity

    astro-ph.CO 2024-02 unverdicted novelty 7.0

    Λ_s VCDM is a predictive model combining Λ_s CDM with VCDM gravity via an auxiliary scalar field and sigmoid-smoothed potentials to enable stable mirror AdS-to-dS transitions with possible transient acceleration.

  3. The impact of Hawking radiation from primordial black holes on recombination and the Hubble tension

    astro-ph.CO 2026-07 conditional novelty 6.0

    PBH evaporation at ΩPBH≈1e-3 ΩC delays recombination (Δz≈64) and boosts CMB-inferred H0 by ~9%, enough to nominally resolve the Hubble tension, though full CMB fits require lower densities.

  4. Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements

    astro-ph.CO 2026-06 conditional novelty 6.0

    A geometric invariance makes the BAO-SN Ω_m gap invariant under sound-horizon rescaling α and requires opposite w(z) deformations for the two datasets, so their combination cannot reach the local H0 value.

  5. Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM

    astro-ph.CO 2025-10 unverdicted novelty 6.0

    Relativistic N-body simulations of Lambda_s CDM produce a redshift-dependent crest in the matter power spectrum ratio, peaking at 20-25% near the transition and leaving a 15-20% uplift at z=0 on group scales.

  6. Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth

    astro-ph.CO 2025-09 accept novelty 6.0

    The correlations between tau_reio and the parameters behind cosmic tensions are not intrinsic, but arise indirectly through networks of other cosmological parameters.

  7. Selection effects in correlated observations with application to distance-ladder observations

    astro-ph.CO 2026-07 conditional novelty 5.0

    Residual correlated-selection effects are weakly detected (1.2–1.9σ) in Cepheid photometry and can shift the distance-ladder Hubble constant down by 0.7–1.1 km/s/Mpc.

  8. The potential broader complex linked to the key Cepheid SV Vul

    astro-ph.SR 2026-07 conditional novelty 5.0

    SV Vul and its host cluster Alicante 13 lie at 2.30 ± 0.13 kpc and may share a common origin with the nearby cluster Liu-Pang 1738.

  9. Hubble tension in k-essence: Evidence for robust tension alleviation

    astro-ph.CO 2026-07 conditional novelty 5.0

    Dilaton and tachyon k-essence models robustly reduce Planck–late-Universe H0 tension to 0.14σ and 0.69σ without dataset-dependent fine-tuning of model parameters.

  10. Cosmological intercept tension

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    Tensions in the supernova intercept a_B at z~0.01 in PantheonPlus and z~0.1 in DES-Y5 point to data systematics or inter-survey inconsistencies rather than new physics, aligning H0 measurements and reducing support fo...

  11. The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch

    astro-ph.GA 2025-03 unverdicted novelty 5.0

    JWST TRGB distances to 10 SN Ia hosts update calibrations for 11 SNe yielding H0 of 68.4-69.6 km/s/Mpc and show modest shifts when combined with prior HST data.

  12. Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension

    astro-ph.CO 2026-07 conditional novelty 4.0

    The SNIa absolute-magnitude tension between the distance ladder (−19.204) and CMB+ΛCDM (−19.430) is independent of late-time expansion history, and DESI's w0–wa dark-energy hints shift H0 by only ~0.3–0.4 km/s/Mpc.

  13. Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation

    astro-ph.CO 2026-07 unverdicted novelty 4.0

    Dynamical dark energy remains preferred across extended models while curvature, neutrino mass and inflation parameters show strong model dependence, with no resolution of the H0 tension.

  14. Cosmological Viability of Exponential Infrared $f(T)$ Gravity

    astro-ph.CO 2026-06 unverdicted novelty 4.0

    Exponential IR f(T) gravity Model I alleviates Hubble tension but is disfavoured by combined Planck/ACT/SPT+DESI+Pantheon+ data; Model II is ruled out because background constraints force unphysical shifts in CMB parameters.

  15. Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference

    astro-ph.CO 2026-06 unverdicted novelty 4.0

    Hybrid redshift model with postulated quantum correction fits Pantheon+SH0ES data to recover Planck-consistent expansion H_Λ and eliminates apparent drift in inferred Hubble parameter across bins.

  16. Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4

    astro-ph.CO 2025-12 unverdicted novelty 4.0

    Local Hubble constant anisotropy in Cosmicflows-4 data is primarily attributed to peculiar velocities and survey structure rather than cosmic-scale isotropy violation, with limited implications for the Hubble tension.

  17. Evaluating Cepheid Metallicity Effect Determinations via IC1613 and Gaia-independent Parallaxes

    astro-ph.SR 2026-06 unverdicted novelty 3.0

    Unifies HST parallaxes to obtain IC1613 distance ~24.39 mag and disfavors large Cepheid metallicity corrections γ(W_VI) of -0.25 or -0.50 mag dex⁻¹ relative to TRGB benchmarks.

  18. Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2

    physics.gen-ph 2026-04 unverdicted novelty 2.0

    MCMC constraints on two Lambda(t) models with DESI DR2, CC, and Pantheon+ data yield H0 ~72.5-73 km/s/Mpc, Omega_m0 near standard values in joint fits, and n~0.3 indicating mild deviation from LambdaCDM.

  19. Fundamental Physics in 2025: Status, Decisive Targets, and Path Forward

    gr-qc 2025-12 unverdicted novelty 2.0

    The review summarizes the baseline SM+GR+Lambda-CDM framework, lists major anomalies and missing pieces, surveys theoretical and experimental approaches, and outlines a staged roadmap organized by decision points.