Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1907.10328.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T05:33:07.847440Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T07:37:44.781723Z
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 8c07330d-abdc-4155-8d4e-3b1c7347b48e · inbound
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T05:33:07.847440Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 84006bc9-afd0-4dfc-a16b-92514903fdb9 · inbound
A "Neural" Riemann solver for Relativistic Hydrodynamics cites this paper.
A "Neural" Riemann solver for Relativistic Hydrodynamics Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 35
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-07T14:28:26.676721Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0082d770-1e14-466f-8d8f-09e191f9d6e8 · inbound
Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers cites this paper.
Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 76
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T08:41:25.398953Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 9d5c3522-b635-4eb6-937f-ca75ebd00c85 · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 77
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:37:44.783249Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 6b61853e-0bd0-49fd-a437-0f8cf499856c · inbound
GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.
GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:35.854356Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 618ae91a-0cfd-4ca9-a0ad-1a739c8dd42a · inbound
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:46.008801Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.