Pith. sign in

Paper Citation Record · LEDGER

The nuclear star cluster of the Milky Way: proper motions and mass

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:0902.3892.

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

pith.paper-citation-record.v1
0902.3892 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T15:58:19.703148Z

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 8d10a550-8220-474e-b258-c847a521ad3a · inbound

Chaotic imprints of dark matter in extreme mass-ratio inspirals cites this paper.

Chaotic imprints of dark matter in extreme mass-ratio inspirals The nuclear star cluster of the Milky Way: proper motions and mass

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-02T21:41:49.302822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T21:41:49.302822Z digest=sha256:97434838802734bc3808d7887436f0dea5d41c96189d95e2074d667d75bf33eb

Observation 5b6025d9-5271-474e-a8cf-01a17f252a22 · inbound

Predicting the unpredictable: binary--single scattering with machine learning cites this paper.

Predicting the unpredictable: binary--single scattering with machine learning The nuclear star cluster of the Milky Way: proper motions and mass

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-01T20:04:56.943327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T20:04:56.943327Z digest=sha256:3075b8cd9065397929b912616542b3fdab299b6f8e3db659f2b415ef1bb6c0a2

Observation 324bf3db-cc1e-4dcb-89f1-cd1552424b1b · inbound

Binary disruptions driven by massive disks around massive black holes cites this paper.

Binary disruptions driven by massive disks around massive black holes The nuclear star cluster of the Milky Way: proper motions and mass

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-01T00:33:40.116006Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:33:40.116006Z digest=sha256:1c292de2ec8e85f662c6bd1b61bfa43b7519056167ff93734bd18d13a7c72db2

Observation 65edc7dd-5b1a-4a68-b5cc-203dec63e287 · inbound

Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 cites this paper.

Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 The nuclear star cluster of the Milky Way: proper motions and mass

Reference 264

Resolution
unresolved
no resolver link, observed 2026-08-11T15:58:19.703148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T15:58:19.703148Z digest=sha256:5ad163703f302daedd6d8ca676d012ed1df1d79e42e1225392a83b3740d90de4