Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The accretion of a solar mass per day by a 17-billion solar mass black hole
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2402.15101.
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 2026-08-08T11:43:23.254830Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T22:32:30.184137Z
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 4f7e0a9e-a711-4b00-bfc8-4b38bc6c58df · inbound
Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors cites this paper.
Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors The accretion of a solar mass per day by a 17-billion solar mass black hole
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T11:43:23.254830Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation db249dce-9432-41d3-93d8-f3363ed36a55 · inbound
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The accretion of a solar mass per day by a 17-billion solar mass black hole
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T22:32:30.188393Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.