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Paper Citation Record · LEDGER

Testing kinematic distances under a realistic Galactic potential

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2403.18000.

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

pith.paper-citation-record.v1
2403.18000 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T11:40:38.179947Z

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
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  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
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 6c3364a5-a00f-4c0e-9b9d-859c9b41fd1e · inbound

Introducing the Rhea simulations of Milky-Way-like galaxies I: Effect of gravitational potential on morphology and star formation cites this paper.

Introducing the Rhea simulations of Milky-Way-like galaxies I: Effect of gravitational potential on morphology and star formation Testing kinematic distances under a realistic Galactic potential

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-09T11:40:38.179947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T11:40:38.179947Z digest=sha256:0798107c92adcb11989f4e2c594b87f2b7cbe0d8c53b94ce0ea7c5a2fd1ff111

Observation 5928e489-16b7-401c-94bb-153de787504b · inbound

A map of the outer gas disk of the Galaxy with direct distances from young stars cites this paper.

A map of the outer gas disk of the Galaxy with direct distances from young stars Testing kinematic distances under a realistic Galactic potential

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T10:21:08.857272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T10:21:08.857272Z digest=sha256:8bbe8b3421872404b1dde3eaa4b9fcf7f30f20db324bd9ba69d68b2b49d535bc

Observation c02bc189-02c2-4f7d-a871-0c9707ae1a73 · inbound

Simulations of gas inflow in the Milky Way I. Stellar-Feedback-Regulated Transport from the Central Molecular Zone to the Circumnuclear disk cites this paper.

Simulations of gas inflow in the Milky Way I. Stellar-Feedback-Regulated Transport from the Central Molecular Zone to the Circumnuclear disk Testing kinematic distances under a realistic Galactic potential

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-05-20T16:28:37.857172Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-20T16:26:41.247111Z digest=sha256:62e108724dca2a566226f94182e72c0e07c501bb00496596a65450a8b983f69d