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Paper Citation Record · LEDGER

Time-Dependent AGN Disc Winds II -- Effects of Photoionization

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2504.00117.

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

pith.paper-citation-record.v1
2504.00117 v1

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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:26:18.035691Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

0
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f8a8b139-b0ab-4cb6-bdf9-230b2c951943 · inbound

Monte-Carlo radiation hydrodynamic simulations of line-driven disc winds: relaxing the isothermal approximation cites this paper.

Monte-Carlo radiation hydrodynamic simulations of line-driven disc winds: relaxing the isothermal approximation Time-Dependent AGN Disc Winds II -- Effects of Photoionization

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-08-06T20:26:24.984611Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-08-06T20:26:18.035691Z digest=sha256:25d4c701a21cd09d9452e1e615b4063527e109fd686a05589e3a42324ea64394

Observation d7643bc7-70ea-423d-b7b6-2f260a2a2c49 · inbound

How massive and clumpy must a quasar wind be to create emission line blueshifts? cites this paper.

How massive and clumpy must a quasar wind be to create emission line blueshifts? Time-Dependent AGN Disc Winds II -- Effects of Photoionization

Reference 85

Resolution
unresolved
no resolver link, observed 2026-07-31T03:00:27.841459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T03:00:27.841459Z digest=sha256:1f9d133011c116b589fc0162de12b0a01359766fe2604937a714ecc9799cba68