Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2409.15439.
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 2026-08-06T18:29:55.755383Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T09:21:20.758295Z
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 147139df-14af-4189-a304-6b073543674a · inbound
Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation cites this paper.
Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:29:55.755383Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 89a62f7f-6de6-4ce3-be85-6cb1794cb2e8 · inbound
Progenitor of the recoiling super-massive black hole RBH-1 identified using HST/JWST imaging cites this paper.
Progenitor of the recoiling super-massive black hole RBH-1 identified using HST/JWST imaging Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T07:54:23.775955Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 854e4833-322f-41cc-9fda-910faadb4b05 · inbound
Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.
Predicting intermediate-mass black hole formation in star clusters with machine learning Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters
Reference 126
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T09:21:20.761130Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.