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Paper Citation Record · LEDGER

Abundances and possible diffusion of elements in M67 stars

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1310.6297.

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

pith.paper-citation-record.v1
1310.6297 v4

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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:04.917851Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T10:57:05.987745Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 72c93218-cddd-4299-ab80-12db99d31c92 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Abundances and possible diffusion of elements in M67 stars

Reference 133

Resolution
verified exact
local_arxiv, observed 2026-08-05T10:57:05.990901Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-05T10:57:04.917851Z digest=sha256:4f2f430522f3958dd841e9b0f88b58eb592d935e2d0fdcda1202185a6e85527b

Observation 6fcd9a69-ee16-45a5-a194-169693fa7403 · inbound

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis cites this paper.

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis Abundances and possible diffusion of elements in M67 stars

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-01T16:32:15.258348Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T16:32:15.258348Z digest=sha256:d4d6f86ec2ecc3e3cba420419ea7e5c022e19d206cb2eaeec551681853339ad4

Observation e8a190ac-7cd5-401b-b281-82ee04b35bbc · inbound

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra cites this paper.

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra Abundances and possible diffusion of elements in M67 stars

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-01T04:28:41.677237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:28:41.677237Z digest=sha256:b3c18fe846ee068841697281eeb011e92e85e3608898a242bfbe662eccc51fee