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Paper Citation Record · LEDGER

A rotating satellite plane around Milky Way-like galaxy from the TNG50 simulation

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2303.00441.

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

pith.paper-citation-record.v1
2303.00441 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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T14:18:33.589836Z

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

2
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 8abadc07-022d-4758-82e3-f89d4bb5f9cb · inbound

The satellite galaxies of the Milky Way and Andromeda cites this paper.

The satellite galaxies of the Milky Way and Andromeda A rotating satellite plane around Milky Way-like galaxy from the TNG50 simulation

Reference 264

Resolution
unresolved
no resolver link, observed 2026-08-08T14:18:33.589836Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T14:18:33.589836Z digest=sha256:e90e002c301c179f912d56757480eb5913c22e7852271265a213c5334b0f5b25

Observation f2ff377a-ce46-45c3-90c2-a9b2ce6e73a6 · inbound

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies cites this paper.

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies A rotating satellite plane around Milky Way-like galaxy from the TNG50 simulation

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-08T22:44:22.863240Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-05-08T07:53:55.768886Z digest=sha256:7c5213d8958245d3cf403e6a562a1e0b008fa0fa435c3a21fde0ffc6db4471f6