Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2003.02279.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T10:21:19.132835Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:26:51.365997Z
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 d9fcf1ed-5f14-4432-98de-8f20b3b366f3 · inbound
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range cites this paper.
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T10:21:19.132835Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 250d0b31-6691-4bb9-adc3-2b700dfb0499 · inbound
Trails of clouds in binary black holes cites this paper.
Trails of clouds in binary black holes Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T06:40:42.157828Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c70f00c0-b656-473f-8954-9c3b88c3d73f · inbound
Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects cites this paper.
Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 157
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T15:00:31.151878Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 862e9634-0406-4179-8ed8-b559e14b9f42 · inbound
A universal framework to identify eccentric binary mergers: GW200105 case study cites this paper.
A universal framework to identify eccentric binary mergers: GW200105 case study Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 83
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T08:53:09.854003Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation c2ec48e7-db64-4e12-b44c-e9ce16db3ab1 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 35
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.367404Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation f1f18933-ded4-4be3-879f-ea00de2bac26 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:30.145225Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.