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Paper Citation Record · LEDGER

AGB stars in the Magellanic Clouds. I. The C/M ratio

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0302051.

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

pith.paper-citation-record.v1
astro-ph/0302051 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T03:55:10.305506Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

107
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 71fc8d65-b52c-400f-9c96-05d3eacfe311 · inbound

Milky Way's warped disc traced by AGB stars cites this paper.

Milky Way's warped disc traced by AGB stars AGB stars in the Magellanic Clouds. I. The C/M ratio

Reference 107

Resolution
verified exact
local_arxiv, observed 2026-06-27T19:01:08.389360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:65350af06157b3d08e94fb35b0b5d338c74780089eb8aa99ff7c2a6daf5016d1

Observation 47945786-2e82-4604-8190-7fcf9a8177bf · inbound

JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 cites this paper.

JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 AGB stars in the Magellanic Clouds. I. The C/M ratio

Reference 33

Resolution
unresolved
no resolver link, observed 2026-07-14T03:55:10.305506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T03:55:10.305506Z digest=sha256:f719774d37b9d8493d585d7b5d22418776a4e5e7e64554788e40fdb154f141c5