Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Active galactic nuclei in four metal-poor dwarf emission-line galaxies
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0807.2029.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:21.000224Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 cd15fcd2-90b5-4766-9fb9-c29a2fb2ae45 · 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 Active galactic nuclei in four metal-poor dwarf emission-line galaxies
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:25:32.783568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1ac175b7-a126-4513-86c0-d252c8ea1a9d · inbound
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.
Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Active galactic nuclei in four metal-poor dwarf emission-line galaxies
Reference 161
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T16:36:21.000224Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.