Paper Citation Record · LEDGER

Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0605132.

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

pith.paper-citation-record.v1
astro-ph/0605132 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T13:20:41.871534Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T02:13:00.302396Z

Reference resolution

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 75095add-3fa5-495d-97ff-a9777f9c3584 · inbound

Applying Liouville's Theorem to Gaia Data cites this paper.

Applying Liouville's Theorem to Gaia Data Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-05-25T11:40:44.118010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation a9d9f354-685b-49c8-a2a9-a83a7c9f846f · inbound

The Formation of Globular Clusters cites this paper.

The Formation of Globular Clusters Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 234

Resolution: unresolved; no resolver link, observed 2026-08-10T13:20:41.871534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6a81b234-7512-4d30-bf7a-b2ede940ba05 · inbound

Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations cites this paper.

Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-07T14:41:51.762977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf0e0906-d6cf-4967-8967-236e05676e75 · inbound

Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs cites this paper.

Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-05-10T12:40:23.753968Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation a7495e81-fb58-463c-8bc0-4ca347f01109 · inbound

Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn cites this paper.

Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-06-27T08:50:46.210015Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 1d54501a-8d21-4e8b-ab65-4e19cde182c6 · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters Resolved Massive Star Clusters in the Milky Way and its Satellites: Brightness Profiles and a Catalogue of Fundamental Parameters

Reference 207

Resolution: verified exact; local_arxiv, observed 2026-06-29T02:13:00.303952Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.