Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/9510080.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T00:25:30.579810Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T17:32:25.283139Z
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 a511f2f4-0b98-4270-849f-b2ed7be2cfec · inbound
Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes cites this paper.
Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines
Reference 175
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T17:32:25.284749Z
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.
Observation 79441beb-263f-4b79-9635-aa0eb39edbba · 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 Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07758e62-1ea1-4017-a4f7-a3c2d79654f8 · inbound
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:25:30.579810Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation abc655e1-da9c-4262-81b9-26e2b0efcb46 · 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 Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:11:53.505858Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.