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Paper Citation Record · LEDGER

The Magellanic Corona and the formation of the Magellanic Stream

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.04368.

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

pith.paper-citation-record.v1
2009.04368 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T20:17:59.043668Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

438
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c208c4ab-19f8-44a4-aa99-39f0a295b009 · inbound

OpenSWI: A Massive-Scale Benchmark Dataset for Surface Wave Dispersion Curve Inversion cites this paper.

OpenSWI: A Massive-Scale Benchmark Dataset for Surface Wave Dispersion Curve Inversion The Magellanic Corona and the formation of the Magellanic Stream

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-05T20:17:59.043668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T20:17:59.043668Z digest=sha256:e98c80e4494886f9d672eb2e2257ee7c2cb9c7a222c04372828fe69c3f1d5f84

Observation 6b6615fe-e75b-4586-8a36-b41fdc89e05f · inbound

Accelerating physics-informed neural networks for full waveform inversion using a hybrid quantum-classical finite-basis architecture cites this paper.

Accelerating physics-informed neural networks for full waveform inversion using a hybrid quantum-classical finite-basis architecture The Magellanic Corona and the formation of the Magellanic Stream

Reference 2

Resolution
verified exact
arxiv_id, observed 2026-06-28T16:22:22.499732Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-28T16:13:21.979966Z digest=sha256:554f072b78af33c249520867c3c33c8b81f68fcea055efee53e9ac0a576c3ba8