Paper Citation Record · LEDGER

The Frequency of Binary Stars in the Core of 47 Tucanae

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0105441.

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

pith.paper-citation-record.v1
astro-ph/0105441 v1

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 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:44.297989Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T08:05:16.230513Z

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 406c98fc-da94-42c9-9116-c2d82937757a · inbound

New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences cites this paper.

New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences The Frequency of Binary Stars in the Core of 47 Tucanae

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-05-15T15:36:12.782179Z

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.

Observation cbaa1e12-4f53-4a41-9aca-91c60317a095 · inbound

A new likely pulsar binary in 47~Tucanae from continuum searches cites this paper.

A new likely pulsar binary in 47~Tucanae from continuum searches The Frequency of Binary Stars in the Core of 47 Tucanae

Reference 47

Resolution: unresolved; no resolver link, observed 2026-07-14T14:19:10.716677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5ec0c66f-801a-42ed-a042-0ab2fd7af6ae · inbound

Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The Frequency of Binary Stars in the Core of 47 Tucanae

Reference 155

Resolution: unresolved; no resolver link, observed 2026-08-07T00:15:44.297989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.