Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A calibrated model for N-body dynamical friction acting on supermassive black holes
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2405.08870.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T23:10:43.904654Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T23:10:53.430894Z
Reference resolution
0 of 0 outbound references displayed
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- 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 05a131eb-449a-4939-95ab-53aafe7e868d · inbound
What drives the growth of black holes: a decade of progress cites this paper.
What drives the growth of black holes: a decade of progress A calibrated model for N-body dynamical friction acting on supermassive black holes
Reference 977
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-06T23:10:53.437233Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 6cccd9ee-9b04-478c-b203-f3182604840a · inbound
RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.
RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime A calibrated model for N-body dynamical friction acting on supermassive black holes
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T03:50:12.525767Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cbd2790b-2ce2-4e8c-8aec-568af0106d9e · inbound
How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations cites this paper.
How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations A calibrated model for N-body dynamical friction acting on supermassive black holes
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:39:45.249980Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.