Paper Citation Record · LEDGER

Do high redshift QSOs and GRBs corroborate JWST?

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2405.19953.

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

pith.paper-citation-record.v1
2405.19953 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:05:41.504730Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

4
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation efcdae4d-dd8a-4975-904a-d4283386b9e8 · inbound

Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample cites this paper.

Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample Do high redshift QSOs and GRBs corroborate JWST?

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T05:05:41.504730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb697a15-3cec-468d-916b-75d01ea80983 · inbound

The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples Do high redshift QSOs and GRBs corroborate JWST?

Reference 115

Resolution: metadata mismatch; arxiv_id, observed 2026-06-27T21:01:15.949974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation ed6ce69b-eadf-4ca7-95d7-52de41f8474f · inbound

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

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements Do high redshift QSOs and GRBs corroborate JWST?

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-07-03T15:38:34.035138Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 2800220f-030b-4634-bdba-0039b02a81d3 · inbound

Redshift-Dependent Intrinsic Dispersion in the Quasar UV/X-ray Luminosity Relation cites this paper.

Redshift-Dependent Intrinsic Dispersion in the Quasar UV/X-ray Luminosity Relation Do high redshift QSOs and GRBs corroborate JWST?

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-07-04T14:19:54.922194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.