Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The nature of massive black hole binary candidates: I. Spectral properties and evolution
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.4941.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.326266Z
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 0f3b8209-7c31-463c-8420-96d1315d3f05 · inbound
Cosmic Pairs: A DESI Census of Dual and Offset AGN as Precursors to Massive Black Hole Binaries cites this paper.
Cosmic Pairs: A DESI Census of Dual and Offset AGN as Precursors to Massive Black Hole Binaries The nature of massive black hole binary candidates: I. Spectral properties and evolution
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:21:00.115001Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2bfe2d47-9397-4b25-bc0d-71e26a9f268a · 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 $z < 0.35$ The nature of massive black hole binary candidates: I. Spectral properties and evolution
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T16:36:20.326266Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.