Pith. sign in

Paper Citation Record · LEDGER

Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2310.18158.

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

pith.paper-citation-record.v1
2310.18158 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:49:07.988302Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T01:39:25.213548Z

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 0f1f8fd0-0347-4f26-b4ec-fbea58050dec · inbound

Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop cites this paper.

Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-11T11:49:07.988302Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T11:49:07.988302Z digest=sha256:f9b106198588402490793163542b2286c29ff8bf004661f147f970c69abee135

Observation b8ae1af9-fd53-4fd3-9e90-80ff2e49d901 · 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 Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-10T13:27:10.047047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T13:27:10.047047Z digest=sha256:fde6379b792f4103d4d66076b699626ed82326036816635cbd055d977947d294

Observation a9bae78e-aa0a-45c2-a25a-1f2f0ed8fcfc · inbound

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 cites this paper.

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-16T23:11:20.924997Z

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=2026-05-16T23:10:51.250004Z digest=sha256:c210b69e8deb4e95d68c58c0e5cdb62d193cb626d8b9a4290865f9ac5d56cb47

Observation a932def2-5b0f-4a7f-a9ee-61ebfc3af234 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 124

Resolution
verified exact
arxiv_id, observed 2026-05-22T09:21:20.944412Z

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=2026-05-22T09:20:09.976842Z digest=sha256:06665f51b41ec692ccd5b11045d232f1722863ffdafbbf888a0fbcd7bbfaaf73

Observation 4f7fd46d-bf67-434f-89ba-52eff56c4bd4 · inbound

Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters cites this paper.

Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 66

Resolution
verified exact
arxiv_id, observed 2026-07-04T01:39:25.216800Z

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=2026-06-26T20:15:37.780290Z digest=sha256:04c6b4ec540de49ae0ef73fa5c50354e51a5dea384d85a10c1baa16cb05268c7