Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1205.5338.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T11:05:41.925725Z
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 c078a616-8969-4223-817d-3d59b72bfebc · inbound
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations cites this paper.
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
Reference 113
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T01:01:26.792212Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 24c726a7-4243-4dc0-a503-ae11906899ef · inbound
Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP cites this paper.
Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
Reference 278
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-01T11:05:41.927083Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.