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Paper Citation Record · LEDGER

The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2303.03791.

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

pith.paper-citation-record.v1
2303.03791 v2

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 2026-08-10T13:27:10.835863Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

3
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 97b50a25-d2ef-462c-a9f5-cff87fbbafdc · inbound

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function

Reference 116

Resolution
unresolved
no resolver link, observed 2026-08-10T13:27:10.835863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T13:27:10.835863Z digest=sha256:b5e00fe161b738fe44f84737e5508b0616f136a3a365d56c72af02ee88626d65

Observation e8b25d0c-0055-4b2f-830c-7de256f2e4e4 · inbound

The Formation of Globular Clusters cites this paper.

The Formation of Globular Clusters The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-10T13:20:41.276349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T13:20:41.276349Z digest=sha256:164d25ef5745e61af1a7b9f2d23738131e2a495cea342fbab589c7bf8f7f080f

Observation c9b61b7b-a28a-455d-ba4c-572e7dc785da · inbound

Dark Star Clusters or Ultra-Faint Dwarf galaxies? Revisiting UMa3/U1 cites this paper.

Dark Star Clusters or Ultra-Faint Dwarf galaxies? Revisiting UMa3/U1 The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-08-05T20:30:22.939422Z

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.

source=pdf_text observed=2026-08-05T20:30:15.368141Z digest=sha256:1e60f5eb93b0ebd6db27315be6f7d7be5e1fcb7d79eaba12545b181b9faee079