Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1705.04734.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.122900Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T13:02:10.520462Z
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 9acfd91e-e501-4c6f-97ea-15cc1b89a1a8 · inbound
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:35:56.122900Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb898c42-81f9-4176-b407-4f74e04b8cf4 · inbound
Population Synthesis of Gravitational Wave Sources cites this paper.
Population Synthesis of Gravitational Wave Sources Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
Reference 152
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T04:41:35.785289Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 850e876d-4587-49c9-aafe-a5b1c6fd4229 · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
Reference 92
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.521782Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.