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Paper Citation Record · LEDGER

In-situ vs accreted Milky Way globular clusters: a new classification method and implications for cluster formation

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2309.15902.

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

pith.paper-citation-record.v1
2309.15902 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 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:21:41.057937Z

measured 0 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
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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 611a4967-6b5e-4430-9518-da5f30daf7f4 · inbound

Updated bounds on ultra-light dark matter from the tiniest galaxies cites this paper.

Updated bounds on ultra-light dark matter from the tiniest galaxies In-situ vs accreted Milky Way globular clusters: a new classification method and implications for cluster formation

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-05T11:31:04.041190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:31:04.041190Z digest=sha256:6289d23e69f6f230f7ee84f0f9b1f630cc76ac47e2f7f43433179a2bba61b69f

Observation 5baf6210-9204-4e8b-9aef-6572179f5fd8 · inbound

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

New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences In-situ vs accreted Milky Way globular clusters: a new classification method and implications for cluster formation

Reference 172

Resolution
verified exact
arxiv_id, observed 2026-05-15T15:36:12.472755Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-15T15:32:23.373591Z digest=sha256:b6d8eec004f15b77b54dfbdfd526479f5b75a02fa8b15c5afd3a058a54cbae09

Observation 33136e92-277b-403b-8ff0-3c3c3f2ceffb · inbound

Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics cites this paper.

Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics In-situ vs accreted Milky Way globular clusters: a new classification method and implications for cluster formation

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-06T16:21:41.057937Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T16:21:41.057937Z digest=sha256:05a65db938b9b0f9d1e7cdf94c2250a95ffc60564c1fdd987e5eee6cc65d4c17