Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2204.09061.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T02:15:29.851550Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:26:51.333118Z
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 dd5f759e-6768-4f90-a2e7-f50f24cd56b9 · inbound
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits cites this paper.
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
Reference 8
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T20:26:51.067438Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation ae7bd88f-6537-4d18-ba63-de0d58dc3a58 · 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 The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.334652Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation b1257dff-6cb4-4cfc-89b5-4fd8821ec74f · 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 The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:29.851550Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.