Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1710.01311.
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 2026-08-14T14:29:00.556836Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T07:37:44.752431Z
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 3dcb2221-cb8e-42f3-a05e-83ce5534946e · inbound
Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity cites this paper.
Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T14:29:00.556836Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fb69410d-0c5d-4eba-b1ba-ecb6a58fd262 · inbound
Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers cites this paper.
Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:29:52.836073Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 33225bda-c9cb-4b5e-b512-be6b166d15b5 · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T07:37:44.753633Z
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.
Observation 60ea3e53-3e70-4d81-a586-1ace7df53bbe · inbound
Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics cites this paper.
Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 100
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T07:16:44.130862Z
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.
Observation f11c944e-bb61-4ee1-86d2-fab9ff7d104e · inbound
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors cites this paper.
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 109
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T05:14:58.841553Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df94fa85-0561-43c8-af7b-96ea9b8fb1a0 · inbound
Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.
Transport Properties of the MRI in Differentially Rotating Neutron Stars Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T14:28:12.574381Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.