Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1611.07028.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T17:13:11.324459Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T05:04:19.212322Z
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 6688a75c-6cf0-433f-bc4c-0293c8171fd2 · inbound
$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer cites this paper.
$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T17:13:11.324459Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3fd32122-6b49-4015-81a8-92cb5b84618a · inbound
Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations cites this paper.
Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T17:11:05.945581Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 396483e2-4985-4f82-8284-34217441dcca · inbound
The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models cites this paper.
The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
Reference 251
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T05:04:19.213847Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation c20c6663-3720-4107-a668-258b570582fb · 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 Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T03:50:05.136577Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.