Paper Citation Record · LEDGER

Do high redshift QSOs and GRBs corroborate JWST?

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:41:23.693241Z

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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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 e26268e6-0616-45ec-9d1b-72757382205b · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Do high redshift QSOs and GRBs corroborate JWST?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.693241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cbdd934-98fe-4e57-9842-d510a3c907d7 · inbound

Can Dark Stars account for the star formation efficiency excess at very high redshifts? cites this paper.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Do high redshift QSOs and GRBs corroborate JWST?

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T20:58:09.328492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-13T06:32:02.005865+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 2026-08-13T06:32:02.005865+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 2026-08-13T06:32:02.005865+00:00.