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Paper Citation Record · LEDGER

Measurement of the expansion rate of the Universe from \gamma-ray attenuation

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.2163.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1305.2163 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T03:39:16.007852Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-15T11:50:20.765756Z

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 188a9ed7-7b52-4544-880b-7c9d859d9edd · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions Measurement of the expansion rate of the Universe from \gamma-ray attenuation

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-05-15T11:50:20.768797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-15T11:50:20.600831Z digest=sha256:edd2bac67b2b3c200275d1c547754c0aa07d6de82cafb8dc63163aec99ad53a2

Observation e225a1ed-8ab7-4e38-b0ac-4f9e7b2eb77d · inbound

Constraining cosmological parameters from very-high-energy $\gamma$-ray attenuation in blazar spectra: Bayesian inference and systematic uncertainties cites this paper.

Constraining cosmological parameters from very-high-energy $\gamma$-ray attenuation in blazar spectra: Bayesian inference and systematic uncertainties Measurement of the expansion rate of the Universe from \gamma-ray attenuation

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-01T03:39:16.007852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T03:39:16.007852Z digest=sha256:2059e677add334df018001bb44fb485d0f28674e509d47ed3495619739c7acab