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Paper Citation Record · LEDGER

Rotating Accretion Flows: From Infinity to the Black Hole

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1206.4059.

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

pith.paper-citation-record.v1
1206.4059 v4

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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:45:37.475826Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

116
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bcdec306-de4e-4d3a-bfd9-59fcd533b631 · inbound

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes cites this paper.

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes Rotating Accretion Flows: From Infinity to the Black Hole

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T11:45:37.475826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T11:45:37.475826Z digest=sha256:2eb3022939a5d720cf61a4227c0b76d7ca850d6755f720d98014cfcea71a13ca

Observation 7a162296-1b81-482a-93ae-82e0d3a5bd24 · inbound

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes cites this paper.

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes Rotating Accretion Flows: From Infinity to the Black Hole

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:21:48.936666Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ce75c18038bcb0f2a3e38e9123bd8e092947639e08da01f6c630b64ed8195fb1