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Paper Citation Record · LEDGER

A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2308.06951.

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

pith.paper-citation-record.v1
2308.06951 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:56:28.753099Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T12:48:11.319841Z

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 fe60571b-0068-4eac-82dc-bdc1573f98dd · inbound

A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant cites this paper.

A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T14:56:28.753099Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:56:28.753099Z digest=sha256:117bc24ce28da73739fc7ab71268b15c49b35e13705598911af730db6e6f0438

Observation 1550733f-95a3-4b33-97ef-422e125813ff · inbound

Deep Learning Calibration of the Quasar X-ray/UV Luminosity Relation for Cosmological Applications cites this paper.

Deep Learning Calibration of the Quasar X-ray/UV Luminosity Relation for Cosmological Applications A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-07-03T12:48:11.321124Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-27T08:47:03.825664Z digest=sha256:a9ddbe12c26a0c3339867d9f2039a8a1b59f31702889ee8d77bd7fc43c9422ef