Paper Citation Record · LEDGER

On the dependence of the iron K-line profiles with luminosity in Active Galactic Nuclei

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9708030.

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

pith.paper-citation-record.v1
astro-ph/9708030 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:11:50.661129Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

163
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9bf8a95b-10b6-4ff4-9fef-4564625d7cb8 · inbound

Accretion of Primordial Black Holes in Stellar Interiors cites this paper.

Accretion of Primordial Black Holes in Stellar Interiors On the dependence of the iron K-line profiles with luminosity in Active Galactic Nuclei

Reference 150

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:22:15.643524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation f6763567-5607-44f5-ae1b-206e327d46b0 · inbound

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region cites this paper.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region On the dependence of the iron K-line profiles with luminosity in Active Galactic Nuclei

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.661129Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.