Paper Citation Record · LEDGER

Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1501.01197.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1501.01197 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:41:37.537411Z

measured 0 of 1 external citation measurements

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
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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 d32dc714-92a9-4cb1-b911-0d52dd53b9eb · inbound

M87: a cosmic laboratory for deciphering black hole accretion and jet formation cites this paper.

M87: a cosmic laboratory for deciphering black hole accretion and jet formation Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach

Reference 284

Resolution: unresolved; no resolver link, observed 2026-08-11T19:13:05.268764Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca217193-a4f4-4cc3-8910-6709651c4fd4 · inbound

Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields cites this paper.

Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T21:41:37.537411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-21T06:32:19.484+00:00.