Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Numerical Simulations of Super-Eddington Accretion Flows
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2408.16856.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:32:50.545544Z
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
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- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 09cc86f8-bf99-482c-857d-2dcabc944073 · inbound
Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum cites this paper.
Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum Numerical Simulations of Super-Eddington Accretion Flows
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:32:50.545544Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation acd38789-fb80-41b7-ade8-d73322b64845 · inbound
A luminous and hot infrared through X-ray transient at a 5 kpc offset from a dwarf galaxy cites this paper.
A luminous and hot infrared through X-ray transient at a 5 kpc offset from a dwarf galaxy Numerical Simulations of Super-Eddington Accretion Flows
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:58:23.577908Z
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 2026-08-20T06:33:59.587034+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 2026-08-20T06:33:59.587034+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.