Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2204.05336.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:55.890720Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T19:46:33.636057Z
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 d131d2d6-0c61-4ef7-81cb-d231eb21054e · inbound
Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories cites this paper.
Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:16:42.108616Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 05db39e9-44b3-481f-8380-7b658ffd337b · inbound
Remnant properties of binary neutron star mergers undergoing prompt collapse cites this paper.
Remnant properties of binary neutron star mergers undergoing prompt collapse Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T14:25:05.961353Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3b0b2fa3-e432-40e4-a93d-5228dba2f007 · inbound
Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring cites this paper.
Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
Reference 30
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T19:46:33.639224Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation c71f22f8-23cd-40a6-9044-d63617c5f69c · inbound
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:20:55.890720Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50b3f06a-dffc-4a46-ad3a-b9ae464989af · inbound
Scalar baryons in neutron stars cites this paper.
Scalar baryons in neutron stars Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:19:49.404009Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.