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Paper Citation Record · LEDGER

Efficiency of Super-Eddington Magnetically-Arrested Accretion

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1508.02433.

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

pith.paper-citation-record.v1
1508.02433 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:53:23.798307Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T00:54:07.192730Z

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 e6567905-e3e6-41f3-98b1-7cf7e5a138aa · inbound

Effects of Bethe-Heitler pair production in ultraluminous X-ray sources cites this paper.

Effects of Bethe-Heitler pair production in ultraluminous X-ray sources Efficiency of Super-Eddington Magnetically-Arrested Accretion

Reference 22

Resolution
malformed identifier
no resolver link, observed 2026-08-05T10:53:23.798307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T10:53:23.798307Z digest=sha256:8265267813288ce8b9c5972733894500c48d63a6c2a526e70197c6c4e6c3a888

Observation e873fb30-575e-4e5a-be6a-999f797d106e · 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 Efficiency of Super-Eddington Magnetically-Arrested Accretion

Reference 177

Resolution
verified exact
local_arxiv, observed 2026-06-30T00:54:07.194210Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f0d997125728ae4677bebb6bf77d924cfa9b0124d26aac83e7c7c5929d9caf22