Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1705.06142.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T00:32:16.779392Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T07:37:45.067933Z
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 753b2923-ac92-4198-a3d5-2032e9673046 · inbound
Science with the Einstein Telescope: a comparison of different designs cites this paper.
Science with the Einstein Telescope: a comparison of different designs Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
Reference 244
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T21:45:18.070711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation eb6bd434-ee31-4d12-90de-a069777b2fd9 · inbound
Superradiant amplification by rotating viscous compact objects cites this paper.
Superradiant amplification by rotating viscous compact objects Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:32:16.779392Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a76aabec-eac3-4eea-b159-7d50c1e0efdb · inbound
Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks cites this paper.
Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
Reference 100
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T14:54:45.323791Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 68c808be-7391-4ffa-ab73-db2484e43bed · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
Reference 121
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T07:37:45.069430Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.