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Paper Citation Record · LEDGER

The Accretion flow in M87 is really MAD

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2201.00512.

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

pith.paper-citation-record.v1
2201.00512 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:18:32.557340Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T12:18:07.471139Z

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 865b8cc6-e172-464d-baf0-337ef9bb7897 · 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 The Accretion flow in M87 is really MAD

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-05T17:13:11.684184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T17:13:11.684184Z digest=sha256:7d5b5fc1bedce8609af150493651eaf45b0ed72b5aaa1623fbaea35d02826a6b

Observation 706e9b1f-842e-41c3-bc77-f8187c0246d1 · inbound

A Jet from a Nearly Dormant Black Hole cites this paper.

A Jet from a Nearly Dormant Black Hole The Accretion flow in M87 is really MAD

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-07-03T12:18:07.475138Z

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=pdf_text observed=2026-06-27T09:00:41.337519Z digest=sha256:770385f80b5e9b93cbd6027e990fd87651caa694c521dc143ab88b461eb453f4

Observation eaf3babc-1d35-4d1e-a510-c1e8c459adf7 · inbound

Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows cites this paper.

Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows The Accretion flow in M87 is really MAD

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T00:18:32.557340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T00:18:32.557340Z digest=sha256:431010d5cc7a06b219c998f1823ff08ff2cf2a6c83982cf69c36a7385a200a5d