Paper Citation Record · LEDGER

A non-axisymmetric potential for the Milky Way disk

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2411.12800.

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

pith.paper-citation-record.v1
2411.12800 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T05:33:55.256147Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T06:16:28.064256Z

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 fc83daa5-aa11-46aa-9630-523a8a10febd · inbound

Signatures of simulated spiral arms on radial actions cites this paper.

Signatures of simulated spiral arms on radial actions A non-axisymmetric potential for the Milky Way disk

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-11T05:33:55.256147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c259dfdb-0a40-485b-aa0e-2d0d9a69c417 · inbound

Using simulation based inference on tidally perturbed dwarf galaxies: the dynamics of NGC205 cites this paper.

Using simulation based inference on tidally perturbed dwarf galaxies: the dynamics of NGC205 A non-axisymmetric potential for the Milky Way disk

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T16:32:33.014130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7800163a-ee24-401a-bcdb-36fc8d3d1414 · inbound

Bar-spiral interaction produces radial migration and star formation bursts cites this paper.

Bar-spiral interaction produces radial migration and star formation bursts A non-axisymmetric potential for the Milky Way disk

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-09T11:39:17.576717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4cc2b82-b506-406f-b2b7-ab877c432e52 · inbound

Deep Potential: Recovering the gravitational potential and local pattern speed in the solar neighborhood with GDR3 using normalizing flows cites this paper.

Deep Potential: Recovering the gravitational potential and local pattern speed in the solar neighborhood with GDR3 using normalizing flows A non-axisymmetric potential for the Milky Way disk

Reference 65

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T20:07:28.782441Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.