Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why are AGN found in High Mass Galaxies?
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:0801.3530.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-10T18:58:57.399936Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-10T23:35:52.148026Z
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 cffaa915-f32d-488c-a507-dd79902c3c91 · inbound
The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels cites this paper.
The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels Why are AGN found in High Mass Galaxies?
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T17:08:57.096480Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.