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Paper Citation Record · LEDGER

A disk instability model for the quasi-periodic eruptions of GSN 069

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2203.12137.

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

pith.paper-citation-record.v1
2203.12137 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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T13:29:43.335109Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T22:39:01.818684Z

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 87714bc5-7766-4a87-bb19-e4abc17a81b8 · inbound

Orbital evolution of asymmetric binaries within accreting environments cites this paper.

Orbital evolution of asymmetric binaries within accreting environments A disk instability model for the quasi-periodic eruptions of GSN 069

Reference 48

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:39:01.819983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-26T23:24:01.303227Z digest=sha256:403b2db34c10a323230a942393a6164b164c48062d3e4f8c43776d2bc847c818

Observation f3b88ee5-390f-4cb6-a4a5-e99d63552748 · inbound

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer cites this paper.

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer A disk instability model for the quasi-periodic eruptions of GSN 069

Reference 166

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:43.335109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:29:43.335109Z digest=sha256:848982e4da4df61a6d069e18df49b39590320c6c22cded5f0bda6507c4d118e4