Pith. sign in

Paper Citation Record · LEDGER

Globular cluster populations and the kinematical fingerprints of minor mergers

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1802.00812.

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

pith.paper-citation-record.v1
1802.00812 v2

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:17:26.696404Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 061088b1-5195-440a-a61e-c8a9554203b2 · inbound

The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc cites this paper.

The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc Globular cluster populations and the kinematical fingerprints of minor mergers

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-07T00:14:13.598033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:14:13.598033Z digest=sha256:10318189a6312c29a482b193229a85f57b2d3d49230910d75c1e2ff10fef95e8

Observation e7861204-e90c-4f25-a015-532b11fd24e5 · inbound

Does IRS13 require an intermediate-mass black hole? cites this paper.

Does IRS13 require an intermediate-mass black hole? Globular cluster populations and the kinematical fingerprints of minor mergers

Reference 196

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.696404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.696404Z digest=sha256:d23731655b3e346031f631284c85e7eb5172796f88c04f52ef31bce55de0d239