Paper Citation Record · LEDGER

Numerical Simulations of Super-Eddington Accretion Flows

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2408.16856.

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

pith.paper-citation-record.v1
2408.16856 v1

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 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T20:03:35.985247Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0b5cea91-296d-4875-aa2f-cd272adf037c · inbound

Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates cites this paper.

Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates Numerical Simulations of Super-Eddington Accretion Flows

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-08T20:03:35.985247Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd77121c-4c61-45c0-b4da-b3d0c2ebee05 · inbound

Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios cites this paper.

Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios Numerical Simulations of Super-Eddington Accretion Flows

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T11:34:29.012222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4d953047-b7e8-4ae1-ab82-1c5478b9d65a · inbound

Do Little Red Dots Vary? cites this paper.

Do Little Red Dots Vary? Numerical Simulations of Super-Eddington Accretion Flows

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T10:54:53.104586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66b7b5de-a44a-4bf8-966b-19e44f544f46 · inbound

Supermassive Black Hole Growth in Massive Galaxies at Cosmic Dawn cites this paper.

Supermassive Black Hole Growth in Massive Galaxies at Cosmic Dawn Numerical Simulations of Super-Eddington Accretion Flows

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T08:39:41.383169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3fd4e0d0-6c03-4745-b6dd-d7d8d03733a0 · inbound

Investigating the Spectral Properties of Dual Nuclei in Galaxy Mergers from the GOTHIC survey: Supermassive Black Hole Growth, metal enrichment and Dual AGN cites this paper.

Investigating the Spectral Properties of Dual Nuclei in Galaxy Mergers from the GOTHIC survey: Supermassive Black Hole Growth, metal enrichment and Dual AGN Numerical Simulations of Super-Eddington Accretion Flows

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-06-26T16:19:34.815323Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 9d98dd43-e60d-427b-90d9-66d122ecc892 · inbound

Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds cites this paper.

Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds Numerical Simulations of Super-Eddington Accretion Flows

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-06-26T01:28:51.357829Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b922b980-5db6-4fcd-b8dd-d1d6e9815de3 · inbound

Strongly Magnetized Super-Eddington Accretion: How Spin and Accretion Rate Regulate Energy Output and Mass Loss cites this paper.

Strongly Magnetized Super-Eddington Accretion: How Spin and Accretion Rate Regulate Energy Output and Mass Loss Numerical Simulations of Super-Eddington Accretion Flows

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-03T01:25:10.525618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.