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Paper Citation Record · LEDGER

Why are optical coronal lines faint in active galactic nuclei?

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2408.15229.

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

pith.paper-citation-record.v1
2408.15229 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 2026-08-04T18:47:40.968844Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a46e8d10-79aa-4884-b3ba-8743c0081f09 · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot Why are optical coronal lines faint in active galactic nuclei?

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-04T18:47:40.968844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:47:40.968844Z digest=sha256:2ea3373630569b8d2ee1cd87c1bba5cfdf334171d7d6c9805ad978f317765e1d

Observation 886980c4-8b83-4392-8790-04508fcac0b3 · inbound

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System cites this paper.

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System Why are optical coronal lines faint in active galactic nuclei?

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-01T17:12:31.496182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T17:12:31.496182Z digest=sha256:0ce91b069efa18907e71c5f5990e2b996a0c4fe6f1e57b6ea2bd2b2a150612be