Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2303.06974.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T04:21:03.803877Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T20:51:50.437504Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 4a06a774-eacc-4676-b4eb-5ce8487d94ee · inbound
Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations cites this paper.
Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T15:36:37.303626Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 195411ff-bd3d-4a19-8b02-aa10c780e421 · inbound
A $\Lambda$CDM Extension Explaining the Hubble Tension and the Spatial Curvature $\Omega_{k,0} = -0.012 \pm 0.010$ Measured by the Final PR4 of the Planck Mission cites this paper.
A $\Lambda$CDM Extension Explaining the Hubble Tension and the Spatial Curvature $\Omega_{k,0} = -0.012 \pm 0.010$ Measured by the Final PR4 of the Planck Mission Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:49:11.823161Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8adc67c2-b182-455e-b497-c9a2661e4166 · inbound
Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations cites this paper.
Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:21:03.803877Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bab6c711-daa7-4f12-b81f-247ee276d653 · inbound
Gravitational particle production, the cosmological tensions and fast radio bursts cites this paper.
Gravitational particle production, the cosmological tensions and fast radio bursts Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T20:51:50.439861Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation e12897d1-e663-4ac7-97f1-c7e570149091 · inbound
Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.
Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Reduced uncertainties up to 43\% on the Hubble constant and the matter density with the SNe Ia with a new statistical analysis
Reference 117
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T12:17:52.503402Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.