Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modified viscosity in accretion disks. Application to Galactic black hole binaries, intermediate mass black holes and AGN
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.09322.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-12T03:29:42.101488Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
39
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6203b2bb-883a-4f19-b7c6-a6069b060449 · inbound
Radiation-pressure instability is an artifact of constant-$\alpha$ closure. Implications for AGN disk tensions cites this paper.
Radiation-pressure instability is an artifact of constant-$\alpha$ closure. Implications for AGN disk tensions Modified viscosity in accretion disks. Application to Galactic black hole binaries, intermediate mass black holes and AGN
Reference 137
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T03:35:19.883150Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 2a6b540b-4a70-47e9-b2ad-0b75bd840153 · inbound
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference Modified viscosity in accretion disks. Application to Galactic black hole binaries, intermediate mass black holes and AGN
Reference 183
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.