Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2211.07158.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T13:31:50.238804Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T13:08:08.583320Z
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 a63cf8f4-750e-4fe8-974d-8359e3bbf8fe · inbound
Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo cites this paper.
Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T13:31:50.238804Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 68e24ccb-ccca-43da-b9cc-5d52ad153dab · inbound
Neutrino pair annihilation driven jets from black-hole torus systems cites this paper.
Neutrino pair annihilation driven jets from black-hole torus systems General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T11:41:25.627528Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00f8d526-2b93-4748-b337-820f30b43660 · inbound
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity cites this paper.
Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:32:50.484430Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7b650dbc-ee94-499d-8263-fe4f8602eadf · inbound
Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.
Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 111
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T15:52:56.742594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28bd05fd-04e7-4766-a952-e70e484970e9 · inbound
The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet cites this paper.
The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-14T17:49:23.372202Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 836be71c-e928-4d01-98c1-13a90a602268 · 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 General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 46
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T09:26:51.299793Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 3ee7174c-2fb0-4def-bd42-2c5f1ecaaf17 · 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 General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:31.360046Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb81a790-a66d-42c3-813f-52f611a78f98 · inbound
Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star cites this paper.
Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
Reference 25
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T13:08:08.584823Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.