Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1501.01197.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T12:45:21.720661Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T00:06:27.775191Z
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 f15d478f-f6ce-4c45-ac56-c83c9d74cb93 · inbound
Universal Radial Scaling of Large-Scale Black Hole Accretion for Magnetically Arrested And Rocking Accretion Disks cites this paper.
Universal Radial Scaling of Large-Scale Black Hole Accretion for Magnetically Arrested And Rocking Accretion Disks Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:45:21.720661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 12664ba8-7a6f-4185-adb1-cc6c673e2e7b · inbound
Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve cites this paper.
Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
Reference 235
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T06:14:29.007321Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bececd51-599f-4b43-9ed1-82c3b99896e6 · inbound
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T06:10:49.074313Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bdec093d-bd85-4dc4-8dd8-1724be321802 · inbound
The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.
The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
Reference 291
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-06T00:06:27.777914Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.