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Paper Citation Record · LEDGER

Magnetic support, wind-driven accretion, coronal heating, and fast outflows in a thin magnetically arrested disc

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2302.10226.

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

pith.paper-citation-record.v1
2302.10226 v2

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:15:05.024749Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T03:23:26.540224Z

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 a311d5a9-a68a-454e-bb2d-ef6c98317be0 · inbound

Polarization Signatures from GRMHD Simulations of Black Hole Accretion cites this paper.

Polarization Signatures from GRMHD Simulations of Black Hole Accretion Magnetic support, wind-driven accretion, coronal heating, and fast outflows in a thin magnetically arrested disc

Reference 32

Resolution
verified exact
arxiv_id, observed 2026-05-15T03:08:58.548432Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-15T03:06:24.087052Z digest=sha256:41c3b39e25ee3d0b27dc5a44bfc3b07e1d3db65980a633eacab6d70dba33cb56

Observation da238e52-0f6d-4e0c-99e0-50e8c7e0956f · inbound

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Magnetic support, wind-driven accretion, coronal heating, and fast outflows in a thin magnetically arrested disc

Reference 107

Resolution
unresolved
no resolver link, observed 2026-08-15T15:15:05.024749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:15:05.024749Z digest=sha256:58a628fb2d3942890e3e8a63945b555eec23a70e905d97004597727ad0c0632f