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Paper Citation Record · LEDGER

Large and complex X-ray time lags from black hole accretion disks with compact inner coronae

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2312.08302.

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

pith.paper-citation-record.v1
2312.08302 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T17:00:46.608239Z

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

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

1
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 dfe7283b-bccd-467c-80ca-a5c519a60c5e · inbound

Quasi-Periodic Oscillations due to radiative feedback mechanism between the disc and corona cites this paper.

Quasi-Periodic Oscillations due to radiative feedback mechanism between the disc and corona Large and complex X-ray time lags from black hole accretion disks with compact inner coronae

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-06T17:00:46.608239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T17:00:46.608239Z digest=sha256:d09100a84ec933b6aea2432fffc469bc5ea12ce31d985a14994c6174d78491b5

Observation 692f514b-d7ed-4121-90ae-d649bdb528bc · inbound

Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles cites this paper.

Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles Large and complex X-ray time lags from black hole accretion disks with compact inner coronae

Reference 162

Resolution
verified exact
arxiv_id, observed 2026-05-21T01:29:21.795909Z

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.

source=arxiv_source observed=2026-05-21T01:25:53.670807Z digest=sha256:e550da6f5b8090e3022c2562a59caf57f33a7fe178de6b2cbd2709efd1ceaf54

Observation 834799b5-45d9-4d78-b64d-0642f2841342 · inbound

Evidence for Millihertz Oscillations in the bright atoll source GX 3+1 cites this paper.

Evidence for Millihertz Oscillations in the bright atoll source GX 3+1 Large and complex X-ray time lags from black hole accretion disks with compact inner coronae

Reference 151

Resolution
metadata mismatch
arxiv_id, observed 2026-07-01T04:15:20.924289Z

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.

source=arxiv_source observed=2026-07-01T04:09:40.495263Z digest=sha256:695d6832a15478f2e858e297a8180e65aa827d0640db89d144bfadf1f636f557