Paper Citation Record · LEDGER

Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:astro-ph/0301402.

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

pith.paper-citation-record.v1
astro-ph/0301402 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T17:13:11.739841Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-06-30T00:54:07.015855Z

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 9753f492-a88c-4488-bd28-5bba16d92e05 · 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 Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 116

Resolution: unresolved; no resolver link, observed 2026-08-05T17:13:11.739841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45db1b07-55cf-420c-8ea6-bddcbba77309 · inbound

Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes cites this paper.

Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 232

Resolution: verified exact; local_arxiv, observed 2026-05-15T05:55:05.206114Z

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 7844bc80-c354-42bc-9c1d-aef98fcd0173 · inbound

Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion cites this paper.

Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 159

Resolution: verified exact; local_arxiv, observed 2026-05-20T04:48:04.651302Z

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 e4900205-1464-4c97-bcc3-f41e1e17d947 · inbound

Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion cites this paper.

Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 159

Resolution: verified exact; local_arxiv, observed 2026-05-21T07:29:47.272377Z

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 b9a6f681-e920-438a-b876-2773d829e374 · inbound

Constraining the jet base emission of M87* with past and future Event Horizon Telescope observations cites this paper.

Constraining the jet base emission of M87* with past and future Event Horizon Telescope observations Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 11

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T06:11:42.929342Z

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 2aa4692f-390b-45c1-9c1e-f66ab135a291 · inbound

Identifying Observational Signatures of Flux Eruption Events in Supermassive Black Hole Accretion Flows with Machine Learning cites this paper.

Identifying Observational Signatures of Flux Eruption Events in Supermassive Black Hole Accretion Flows with Machine Learning Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-06-30T00:54:07.017195Z

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 3e34c745-85bc-4fbf-83a9-9d72c3b0c5ce · inbound

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra cites this paper.

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T01:57:42.506091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.