Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1506.05234.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T04:25:34.562461Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T18:35:58.611736Z
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 ccc8ffae-9ef6-4252-89a5-89852c786631 · inbound
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range cites this paper.
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
Reference 186
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T10:21:19.544214Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 60ca8bf9-adfc-4b35-b361-e270d8ba0eaa · inbound
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:27:10.259799Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5f78645-93c3-4a9c-9daf-078d563805ca · inbound
Evolution of a black hole cluster in full general relativity cites this paper.
Evolution of a black hole cluster in full general relativity MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:25:34.562461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c6b15d59-45ad-4c9b-9db7-0cfa0b6ba68a · inbound
Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters cites this paper.
Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
Reference 27
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T18:35:58.615305Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation f2847956-c0ae-4bc9-bf19-eb989fc9f711 · inbound
Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars cites this paper.
Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
Reference 3
- Resolution
- metadata mismatch
- doi, observed 2026-05-09T02:16:27.877655Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.