Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
What broad emission lines tell us about how active galactic nuclei work
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0908.0386.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:33:47.702343Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-12T03:38:27.687542Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 ad22197b-df74-4136-ae2f-6d2fe1f4248a · inbound
The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles cites this paper.
The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles What broad emission lines tell us about how active galactic nuclei work
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:33:47.702343Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd16b63a-ae97-417b-a552-b54fb6b21e59 · 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 What broad emission lines tell us about how active galactic nuclei work
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T18:47:40.941208Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 36b10daa-fb43-4d42-b48c-3015d580fb69 · inbound
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference What broad emission lines tell us about how active galactic nuclei work
Reference 179
- Resolution
- verified exact
- local_arxiv, observed 2026-07-12T03:38:27.689617Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.